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Published online by Cambridge University Press:  27 September 2017

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Part XI
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International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 413 - 431
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Copyright © United States Naval Observatory 1992

References

Aarseth, S. and Lecar, M. 1975, Computer simulations of stellar systems, Ann. Rev. Astr. Ap., 13, 1.Google Scholar
Abies, J. G., Jacka, C. E., McConnell, D., Hamilton, P. A., McCulloch, P. M., and Hall, P. J. 1988. IAU circular 4602.Google Scholar
Abies, J. G., McConnell, D., Jacka, C. E., McCulloch, P. M., Hall, P. J., and Hamilton, P. A. 1989, A millisecond pulsar in a 32-minute binary orbit, Nature, 342, 158–161.Google Scholar
Alekseev, J. I. and Dobysh, G. I. 1989, Multichannel pulsar receiver, FIAN Transactions, 199, 118.Google Scholar
Allakhverdiyev, A. O., Guseiˇnov, O. H., and Yusifov, I. M. 1987, spatial distribution of pulsars and supernova remnants, Aust. J. Phys., 40, 837–845.Google Scholar
Alpar, A., Brinkmann, W., Kiziloğlu, U., Öelman, H., and Pines, D. 1987, A search for X-ray emission from a nearby pulsar PSR 1929+10, Astr. Astrophjys., 177, 101–104.Google Scholar
Alsop, M. A. and Sauls, J. A. 1988, On the dynamical coupling between the superfluid interior and the crust of a neutron star, Astrophys. J., 327, 723–725.Google Scholar
Anawalt, R. A. and Boksenberg, A. 1989, The Astronomical Almanac 1989, (Washington D. C.: U. S. Government Printing Office).Google Scholar
Anderson, S., Kulkarni, S., Prince, T., and Wolszczan, A. 1989. IAU circular 4819.Google Scholar
Anderson, S., Kulkarni, S., Prince, T., and Wolszczan, A. 1990a. IAU circular 5013.Google Scholar
Anderson, S. B., Gorharn, P. W., Kulkarni, S. R., Prince, T. A., and Wolszczan, A. 1990b, Discovery of two radio pulsars in the globular cluster M15, Nature, 346, 42–44.Google Scholar
Andreev, A. V., Emelyanov, V. I., and Ilyinski, Y. A. 1988, Cooperative Phenomena in Optics, (Moscow: Nauka).Google Scholar
Andriesse, C. D. 1980, Josephson pulsars, Astrophys. Space Sci., 70, 173–178.Google Scholar
Ardavan, H. 1981, Is the light cylinder the site of emission in pulsars?, Nature, 289, 44.Google Scholar
Ardavan, H. 1989, The light cylinder catastrophe, Proc. Roy. Soc. London, 424, 113.Google Scholar
Ardavan, H. 1991a, Asymptotic analysis of the radiation by quadrupole sources in supersonic rotor acoustics, J. Fluid Mech., submitted.Google Scholar
Ardavan, H. 1991b, The breakdown of the linearized theory and the role of quadrupole sources in transonic rotor acoustics, J. Fluid Mech., 226, 591.Google Scholar
Argyle, E. and Gower, J. F. R. 1972, The pulse-height distribution for NP 0532, Astrophys. J.. 175, L89–L91.Google Scholar
Armstrong, J. W. 1984, Interstellar scintillations and ultra-low-frequency gravitational wave observations, Nature, 307, 527.Google Scholar
Arnett, W. D., Bahcall, J. N., Kirshner, R. P., and Woosley, S. E. 1989, Supernova 1987A, Ann. Rev. Astr. Ap., 27, 629.Google Scholar
Arnett, W. D. and Bowers, R. L. 1977, A microscopic interpretation of neutron star structure, Astrophys. J. Supp. Series, 33, 415–436.Google Scholar
Arons, J. 1979, Some problems of pulsar physics, or, I'm madly in love with electricity, Space Sci. Rev., 24, 437–510.Google Scholar
Arons, J. 1981a, Pair creation above pulsar polar caps: Steady flow in the surface acceleration zone, Astrophys. J., 248, 1099–1116.Google Scholar
Arons, J. 1981b, Pulsar theory: Particle acceleration and photon emission in the polar flux tube, in Proc. International Summer School and Workshop on Plasma Physics, ed. Guyenne, T. D., volume ESA SP-161, (Paris: European Space Agency), 273–280.Google Scholar
Arons, J. 1981c, The slot gap model of pulsars, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 69–86.Google Scholar
Arons, J. 1983a, Electron-positron pairs in radio pulsars, in Proc. Workshop on Electron-Positron Pairs in Astrophysics, ed. Burns, M. L., Harding, A. K., and Ramaty, R., (New York: American Institute of Physics), 163.Google Scholar
Arons, J. 1983b, On the magnetization and origin of the millisecond pulsar PSR 1937+214, Nature, 302, 301–305.Google Scholar
Arons, J. 1983c, Pair creation above pulsar polar caps: Geometrical structure and energetics of slot gaps, Astrophys. J., 266, 215–241.Google Scholar
Arons, J. and Barnard, J. J. 1983, Are pulsars externally triggered?, J. Astron. and Astrophys. (India), 4, 191–196.Google Scholar
Arons, J. and Barnard, J. J. 1986, Wave propagation in pulsar magnetospheres: Dispersion relations and normal modes of plasmas in superstrong magnetic fields, Astrophys. J., 302, 120–137.Google Scholar
Arons, J., Hoshino, M., and Gallant, Y. A. 1990, Sychrotron instabilities, absorption and suprathermal particle acceleration in relativistic, magnetosonic shock waves, Astrophys. J., (submitted).Google Scholar
Arons, J., Norman, C. A., and Max, C. E. 1977, Electromagnetic parametric instabilities in an ultrarelativistic plasma, Phys. Fluids, 20, 1302.Google Scholar
Arons, J. and Scharlemann, E. T. 1979, Pair formation above pulsar polar caps: Structure of the low altitude acceleration zone, Astrophys. J., 231, 854–879.CrossRefGoogle Scholar
Artyuch, V. S., Pynza'r, A. V., Smirnova, T. V., and Udal'tzov, V. A. 1984, The determination of the distance to PSR 1937+214, Astron. Zh., 61, 515.Google Scholar
Aschenbach, B. and Brinkman, W. 1975, A model of the x-ray structure of the Crab nebula, Astr. Astrophys., 41, 147.Google Scholar
Ashworth, M., Lyne, A. G., and Smith, F. G. 1983, The 1.5 ms pulsar PSR 1937+21, Nature, 301, 313–314.Google Scholar
Asséo, E., Kennel, K. F., and Pellat, R. 1978, Synchrocompton radiation damping of relativistically strong linearly polarized plasma waves, Astr. Astrophys., 65, 401.Google Scholar
Asséo, E., Pellat, R., and Rosado, M. 1980, Pulsar radio emission from beam plasma instability, Astrophys. J., 239, 661–670.Google Scholar
Asséo, E., Pellat, R., and Sol, H. 1981, Pulsar radio emission and bunching mechanisms, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 111–113.Google Scholar
Asséo, E., Pellat, R., and Sol, H. 1983, Radiative or two stream instability as a source for pulsar radio emission, Astrophys. J., 266, 201–214.Google Scholar
Asséo, E., Pelletier, G., and Sol, H. 1990, A nonlinear radio pulsar emission mechanism, Mon. Not. R. astr. Soc., 247, 529–548.Google Scholar
Baars, J. W. M., Genzel, R., Pauliny-Toth, I. I. K., and Witzel, A. 1977, The absolute spectrum of Cas A; An accurate flux density scale and a set of secondary calibrators, Astr. Astrophys., 61, 99–106.Google Scholar
Backer, D. C. 1970, Correlation of subpulse structure in a sequence of pulses from pulsar PSR 1919+21, Nature, 227, 692–695.Google Scholar
Backer, D. C. 1971, Radio intensity fluctuations in pulsars. PhD thesis, Cornell University.Google Scholar
Backer, D. C. 1973, Pulsar fluctuation spectra and the generalized drifting subpulse phenomenon, Astrophys. J., 182, 245–276.Google Scholar
Backer, D. C. 1976, Pulsar average wave forms and hollowcone beam models, Astrophys. J., 209, 895–907.Google Scholar
Backer, D. C. 1987, Millisecond pulsar surveys, in IAU Symposium No. 125: The origin and evolution of neutron stars, ed. Helfand, D. J. and Huang, J. -H., (Dordrecht: D. Reidel), 13–21.Google Scholar
Backer, D. C., Boriakoff, V., and Manchester, R. N. 1973, Wide integrated pulse profiles of pulsars, Nature Phys. Sci., 234, 77.Google Scholar
Backer, D. C. and Rankin, J. M. 1980, Statistical summaries of polarized pulsar radiation, Astrophys. J. Supp. Series, 42, 143–173.Google Scholar
Backus, P. R. 1981, A study of pulsar evolution through timing and single pulse observations. PhD thesis, The University of Massachusetts.Google Scholar
Backus, P. R. and Gilbert, F. 1961, Proc. Nat. Acad. Sci., 47, 362.Google Scholar
Bailes, M. 1988, Geodetic precession in binary pulsars, Astr. Astrophys., 202, 109–112.Google Scholar
Bailes, M. 1989, The origin of pulsar velocities and the velocity-magnetic moment correlation, Astrophys. J., 342, 917–927.Google Scholar
Bailes, M., Manchester, R. N., Kesteven, M. J., Norris, R. P., and Reynolds, J. E. 1989, The proper motion of the Vela pulsar, Aatrophys. J., 343, L53–L55.Google Scholar
Bailes, M., Manchester, R. N., Kesteven, M. J., Norris, R. P., and Reynolds, J. E. 1990, The parallax and proper motion of PSR 1451-68, Nature, 343, 240–241.Google Scholar
Baranov, V. B. and Krasnobaev, K. B. 1986, Hydrodynamic Theory of Cosmic Plasma, (Moscow: Nauka Press).Google Scholar
Bardeen, J. M., Press, W. H., and Teukolsky, S. A. 1972, Rotating black holes: Locally non rotating frames, energy extraction, and scalar synchrotron radiation, Astrophys. J., 178, 347–369.Google Scholar
Barker, B. M. and O'Connell, R. F. 1975a, Phys. Rev., 12, 329.Google Scholar
Barker, B. M. and O'Connell, R. F. 1975b, Relativistic effects in the binary pulsar PSR 1913+16, Astrophys. J., 199, L25–L26.Google Scholar
Barnard, J. J. 1986, Probing the magnetic field of radio pulsars: A reexamination of polarization position angle swings, Astrophys. J., 303, 280–291.Google Scholar
Barnard, J. J. and Arons, J. 1986, Wave propagation in pulsar magnetospheres: Refraction of rays in the open flux zone, Astrophys. J., 302, 138–162.Google Scholar
Bartel, N. 1981, Evidence for ultra broad band absorption of radio emission in the pulsar magnetosphere, Astr. Astrophys., 97, 384–387.Google Scholar
Bartel, N. and Hankins, T. H. 1982, 100-nanosecond time resolution observations of PSR 1133+16, Astrophys. J., 254, L35–L39.Google Scholar
Bartel, N., Kardashev, N. S., Kuz'min, A. D. Nikolaev, N. Y., Popov, M. V., Sieber, W., Smirnova, T. V., Soglasnov, V. A., and Wielebineki, R. 1981, Simultaneous two-station single pulse observations of radio pulsars over a broad frequency range: I. With particular reference to PSR 0809+74, Astr. Astrophys., 93, 85–92.Google Scholar
Bartel, N., Morris, D., Sieber, W., and Hankins, T. H. 1982, The mode-switching phenomenon in pulsars, Astrophys. J., 258, 776–789.Google Scholar
Bartel, N., Sieber, W., and Graham, D. A. 1980, The millisecond intensity variation in the emission of radio pulsars, Astr. Astrophys., 87, 282–291.Google Scholar
Bash, F. N., Bozyan, F. A., and Torrance, G. W. 1970, Observations of CP 1919 and NP 0532 at 38 MHz, Astrophys. Lett., 7 N1, 39–44.Google Scholar
Baym, G., Pethick, C., and Pines, D. 1969, Electrical conductivity of neutron star matter, Nature, 224, 673.Google Scholar
Baym, G., Pethick, C., and Sutherland, P. 1971, The ground state of matter at high densities: Equation of state and stellar models, Astrophys. J., 170, 299–317.Google Scholar
Begelman, M. C. and Kirk, J. 1990, Shock drift particle acceleration in superluminal shocks: A model for hotspots in extragalactic sources, Astrophys. J., 353, 66–80.Google Scholar
Bell, A. R. 1978, The acceleration of cosmic rays in shock fronts, Mon. Not. R. astr. Soc., 182, 147.Google Scholar
Belyaev, S. T. and Budker, G. K. 1956, Dokl. Akad. Nauk. SSSR, 107, 807.Google Scholar
Benford, G. and Buschauer, R. 1977, Coherent pulsar radio emission by antenna mechanisms: General theory, Mon. Not. R. astr. Soc., 179, 189.CrossRefGoogle Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1983a, Soviet Phys. JETP, 85, 235.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1983b, Electrodynamics of a pulsar magnetosphere, Soviet Phys. JETP, 85, 401–433.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1984, Spin-down of pulsars by the current: Comparison of theory with observations, Astrophys. Space Sci., 102, 301–326.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1986a, Physics of pulsar magnetospheres, Soviet Phys. Usp., 29, 946.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1986b, Theory of the radio emission of pulsars, Astrophys. Space Sci., 146, 205.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1987, Permittivity of a weakly inhomogeneous plasma, Soviet Phys. JETP, 92, 1277.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1988a, Generation of radio waves in a pulsar magnetosphere, Sov. Astron. Lett., 14, 93.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1988b, Generation of the radio emission in the pulsar magnetosphere, Pis'ma v Astron. Zh., 14, 224.Google Scholar
Beskin, V. S., Gurevich, A. V., and Istomin, Y. N. 1988c, Theory of the radio emission of pulsars, Astrophys. Space Sci., 146, 205–281.Google Scholar
Bhatia, V. B., Chopra, N., Mujumdar, B., and Panchapakesan, N. 1988, Dependence of pulsar characteristics on the spacetime metric, Astrophys. J., 326, 63–69.Google Scholar
Bhatia, V. B., Chopra, N., and Panchapakesan, N. 1988, The effect of photon capture and field ionization on high magnetic field pulsars, Astrophys. Space Sci., 150, 181–188.Google Scholar
Bhattacharya, D. 1987, The influence of pulsars on supernova remnants. PhD thesis, Indian Institute of Science, Bangladore.Google Scholar
Bhattacharya, D. 1989, The decay of neutron star magnetic fields, in X-ray Binaries, Proc. 23rd ESLAB Symp., ed. Hunt, J. and Battrick, B., (Noordwijk, The Netherlands: ESA), 179.Google Scholar
Bhattacharya, D. 1990a, The evolution of the magnetic fields of neutron stars: An observational overview, in Condensed Matter Properties of Neutron Stars, ed. Srinivasan, G., (Singapore: World Scientific).Google Scholar
Bhattacharya, D. 1990b, Thermal field growth in neutron stars: An alternative to ‘injection’?, in Neutron Stars and Their Birth Events, ed. Kundt, W., (Dordrecht: Kluwer Academic Publishers), 133.Google Scholar
Bhattacharya, D. 1992, The evolution of the magnetic fields of neutron stars, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 27–34.Google Scholar
Bhattacharya, D. and Shukre, C. S. 1985, Has the Crab pulsar magnetic field grown after its birth?, J. Astrophys. Astr., 6, 233.Google Scholar
Bhattacharya, D. and Srinivasan, G. 1986, On the implication of the recently discovered 5 millisecond binary pulsar PSR 1855+09, Curr. Sci., 55, 327.Google Scholar
Bhattacharya, D. and van den Heuvel, E. P. J. 1991, The formation and evolution of binary and millisecond radio pulsars, Phys. Rep., 203, 1–124.Google Scholar
Bhattacharya, D. and Verbunt, F. 1990, Radio pulsars and the scale height of ionized hydrogen, Astr. Astrophys. submitted.Google Scholar
Bhattacharya, D. and Verbunt, F. 1990, Radio pulsars and the scale height of ionized hydrogen, Astr. Astrophys. submitted.Google Scholar
Biggs, J. D. 1986, A study of the individual pulses from southern radio pulsars. PhD thesis, University of Sydney.Google Scholar
Biggs, J. D. 1990a, Main pulse-interpulse correlation and mode changing in PSR 1055-52, Mon. Not. R. astr. Soc., 246, 341–348.Google Scholar
Biggs, J. D. 1990b, Meridional compression of radio pulsar beams, Mon. Not. R. astr. Soc., 245, 514.Google Scholar
Biggs, J. D., Hamilton, P. A., McCulloch, P. M., and Manchester, R. N. 1985a, The drifting subpulses of pulsar 0148-06, Mon. Not. R. astr. Soc., 214, 47P.Google Scholar
Biggs, J. D., Lyne, A. G., Hamilton, P. A., McCulloch, P. M., and Manchester, R. N. 1988, A search for interpulses from southern pulsars, Mon. Not. R. astr. Soc, 235, 255–260.Google Scholar
Biggs, J. D., Lyne, A. G., Manchester, R. N., and Ashworth, M. 1990. IAU circular 4988.Google Scholar
Biggs, J. D., McCulloch, P. M., Hamilton, P. A., and Manchester, R. N. 1987, The drifting subpulses of pulsar 0818-13, Mon. Not. R. astr. Soc., 228, 119.Google Scholar
Biggs, J. D., McCulloch, P. M., Hamilton, P. A., Manchester, R. N., and Lyne, A. G. 1985b, A study of PSR 0826-34 — a remarkable pulsar, Mon. Not. R. astr. Soc., 215, 281–294.Google Scholar
Birdsall, C. and Langdon, A. B. 1985, Plasma Physics via Computer Simulation, (New York: McGraw-Hill).Google Scholar
Bisnovatyi-Kogan, G. S. 1979, Rivista del Nuovo Cimento. 2, 1.Google Scholar
Bisnovatyi-Kogan, G. S. 1989, Two generations of low-mass x-ray binaries and recycled radio pulsars, Astrofizica, 31, 567–577.Google Scholar
Bisnovatyi-Kogan, G. S. 1990, Recycled pulsars, Astrofizica, 32(1), 193–194.Google Scholar
Bisnovatyi-Kogan, G. S. and Komberg, B. V. 1974, Pulsars and close binary systems, Sov. Astron., 18, 217.Google Scholar
Bisnovatyi-Kogan, G. S. and Romanova, M. M. 1983, X-ray burster sources: Their origin and evolution, Astron. Zh., 60, 900–908.Google Scholar
Bjö;rnsson, C. I. 1984, Pulsar polarization as a direct consequence of the emission process, Mon. Not. R. astr. Soc., 208, 293–307.Google Scholar
Blaauw, A. 1985, The progenitors of the local pulsar population, in Birth and Evolution of Massive Stars and Stellar Groups, ed. Boland, W. and van Woerden, H., (Dordrect: D. Reidel), 211–224.Google Scholar
Blair, D. G. and Candy, B. N. 1989, The evolution of pulsars, in Timing Neutron Stars, (NATO ASI series), ed. Ogelman, H. and Heuvel, E. P. J. van den, (Dordrecht: Kluwer Acedemic Publishers), 609–625.Google Scholar
Blandford, R. D. 1975, Amplification of radiation by relativistic particles in a strong magnetic field, Mon. Not. R. astr. Soc., 170, 551.Google Scholar
Blandford, R. D., Applegate, J. H., and Hernquist, L. 1983, Thermal origin of neutron star magnetic fields, Mon. Not. R. astr. Soc., 204, 1025–1048.Google Scholar
Blandford, R. D., Narayan, R., and Romani, R. W. 1984, Arrival-time analysis for a millisecond pulsar, J. Astrophys. Astr., 5, 369–388.Google Scholar
Blandford, R. D. and Romani, R. W. 1988, On the interpretation of pulsar braking indices, Mon. Not. R. astr. Soc., 234, 57P.Google Scholar
Blaskiewicz, M., Cordes, J. M.. and Wasserman, I. 1991, A relativistic model of pulsar polarization, Astrophys. J., 370, 643–669.Google Scholar
Blinnikov, S. I., Novikov, I. D., Perevodchikova, T. V., and Polnarev, A. G. 1984, On the possibility of a neutron star explosion in a close binary, Astron. Zh., 10, 422–428.Google Scholar
Blondin, J. M. and Freese, K. 1986, Is the 1.5 ms pulsar a young neutron star?, Nature, 323, 786–788.Google Scholar
Bogovalov, S. V. 1989, Plasma ejection by pulsars, Pis'ma v Astron. Zhurnal, 15, 1081. (in Russian).Google Scholar
Bogovalov, S. V. 1990, Particle acceleration and gamma-ray production near the light cylinder of an axisymmetric rotator, Sov. Astron. Lett., 16, 844–853.Google Scholar
Bogovalov, S. V. 1992, An analytical solution of the problem of plasma ejection from the magnetosphere of an axisymmetric rotator, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 246–248.Google Scholar
Bogovalov, S. V. and Kotov, Y. D. 1988, Physics of the neutron stars, in Pulsars and Bursters, 91.Google Scholar
Bolotovskii, B. M. and Ginzburg, V. L. 1972, The Vavilov-Cherenkov effect and the Doppler effect in the motion of sources with superluminal velocity in vacuum, Soviet Phys. Usp., 15, 184. in Russian.Google Scholar
Bonin, K. D., McDonald, K. T., Russell, D. P., and Flanz, J. B. 1986, Observation of interference between Cerenkov and sychrotron radiation, Phys. Rev. Lett., 57, 2264.Google Scholar
Boriakoff, V. 1973. Pulsar radio frequency observations with a digital pulsar processor. Technical Repor. 38, NAIC Publication, Arecibo, Puerto Rico.Google Scholar
Boriakoff, V. 1974, A digital pulsar processor, Astr. Astrophys. Suppl. Ser., 15, 479–481.Google Scholar
Boriakoff, V. 1976, Pulsar AP 2016+28: High frequency periodicity in the pulse microstructure, Astrophys. J., 208, L43–L46.Google Scholar
Boriakoff, V. 1983, On the radio pulse emission mechanism of PSR 1133+16: Simultaneous dual-frequency high time resolution observations, Astrophys. J., 272, 687.Google Scholar
Boriakoff, V., Buccheri, R., and Fauci, F. 1983, Discovery of a 6.1-ms binary pulsar, PSR 1953+29, Nature, 304, 417.Google Scholar
Boriakoff, V., Buccheri, R., Fauci, F., Turner, K., and Davis, M. M. 1984, in Birth and Evolution of Neutron Stars: Issues Raised by Millisecond Pulsars, ed. Reynolds, S. P. and Stinebring, D. R., (Green Bank, W. Va: National Radio Astronomy Observatory), 24.Google Scholar
Boriakoff, V. and Ferguson, D. C. 1981, Microstructure cross-correlation in pulses simultaneously observed at frequencies separated by up to 1 GHz, in Pulsars, 13 Years of Research on Neutron Stars, FA U Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 191–196.Google Scholar
Brinkmann, W. and Ögelman, H. 1987, Soft X-rays observations of radio pulsar PSR 1055-52, Astr. Astrophys., 182, 71–74.Google Scholar
Bruck, Y. M. 1987, Decametric emission by pulsars, Aust. J. Phys., 40, 861.Google Scholar
Bruck, Y. M. and Ulyanov, O. M. 1992, Observations of PSR 0823+26 and PSR 0943+10 in the decameter band, in The Magneto spheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 183–185.Google Scholar
Bruck, Y. M. and Ustimenko, B. Y. 1973, Decametric pulsed radioemission from PSR 0809, PSR 1133, and PSR 1919, Nature Phys. Sci., 242, 58.Google Scholar
Bruck, Y. M. and Ustimenko, B. Y. 1976, Decametric radio emission from four pulsars, Nature, 260, 766.Google Scholar
Bruck, Y. M. and Ustimenko, B. Y. 1977a, The interpulse radio-emission of PSR 1919+21 at the frequencies 16.7-38 M Hz, Astrophys. Space Sci., 51, 225–227.Google Scholar
Bruck, Y. M. and Ustimenko, B. Y. 1977b, Some features of the pulsed radiation from the pulsar 1919+21 at 16.7-38MHz, Astrophys. Space Sci., 49, 349–366.Google Scholar
Bruck, Y. M. and Ustimenko, B. Y. 1978, Determination of pulsed signal energy of unknown waveform in the presence of noise, Preprint. 101, IRE Ac. Sci. Ukr. SSR. Kharkov.Google Scholar
Bruck, Y. M. and Ustimenko, B. Y. 1979, The interpulse emission structure in pulsars, Astr. Astrophys., 80, 170.Google Scholar
Buccheri, R. et al.. 1983, Search for pulsed gamma-ray emission from radio pulsars in the COS-B data, Astr. Astrophys., 128, 245.Google Scholar
Buchler, J. R. and Barkat, Z. 1971, Clustering of nucleons in low-density neutron star matter, Astrophys. Lett., 7, 167–170.Google Scholar
Buneman, O. 1959, Dissipation of currents in ionized media, Phys. Rev., 115, 503–517.Google Scholar
Buschauer, R. and Benford, G. 1976, General theory of coherent curvature radiation, Mon. Not. R. astr. Soc., 177, 109.Google Scholar
Buschauer, R. and Benford, G. 1978, Physical mechanism of the Goldreich-Keeley radiative instability, Mon. Not. R. astr. Soc., 185, 493.Google Scholar
Buschauer, R. and Benford, G. 1980, Narrowband versus broadband emission processes in pulsars, Mon. Not. R. astr. Soc., 190, 945–959.Google Scholar
Buschauer, R. and Benford, G. 1983, Relativistic coherent curvature radiation, Astr. Astrophys., 118, 358.Google Scholar
Buti, B. 1962, Plasma oscillations and Landau damping in a relativistic gas, Phys. Fluids, 5(1), 1.Google Scholar
Camenzind, M. 1990, 2D relativistic pulsar winds from rapidly rotating neutron stars, in Neutron Stars and Their Birth Events, ed. Kundt, W., (Dordrecht: Kluwer Academic Publishers), 139–177.Google Scholar
Candy, B. N. and Blair, D. G. 1983, The evolution of radio pulsars, Mon. Not. R. astr. Soc., 205, 281.Google Scholar
Candy, B. N. and Blair, D. G. 1986, The evolution of radio pulsars, Astrophys. J., 307, 535–539.Google Scholar
Canuto, V. and Ventura, J. 1972, Quantum theory of the dielectric constant of a magnetized plasma and astrophysical applications I. Theory, Astrophys. Space Sci., 18, 104.Google Scholar
Carroll, B. W., Zweibel, E. G., Hansen, C. J., McDermott, P. N., Savedoff, M. P., Thomas, J. H., and Van Horn, H. M. 1986, Oscillation spectra of neutron stars with strong magnetic fields, Astrophys. J., 305, 767–783.Google Scholar
Carter, B. and Quintana, H. 1973, Neutron star moment of interia: Theoretical implications of the observational data, Astrophys. Lett., 14, 105–109.Google Scholar
Chandrasekhar, S. 1969, Ellipsoidal figures of equilibrium, (New Haven, Conn.: Yale Univ. Press).Google Scholar
Cheng, A. F. 1985, Interstellar grains and current flow in pulsar magnetospheres, Astrophys. J., 299, 917–924.Google Scholar
Cheng, A. F. and Helfand, D. J. 1983, X-rays from radio . pulsars: The detection of PSR 1055—52, Astrophys. J., 271, 271–282.Google Scholar
Cheng, A. F. and Ruderman, M. A. 1977a, Bunching mechanism for coherent curvature radiation in pulsar magnetospheres, Astrophys. J., 212, 800–806.Google Scholar
Cheng, A. F. and Ruderman, M. A. 1977b, Pair-production discharges above pulsar polar caps, Astrophys. J., 214, 598–606.Google Scholar
Cheng, A. F. and Ruderman, M. A. 1979, A theory of subpulse polarization patterns from radio pulsars, Astrophys. J., 229, 348–360.Google Scholar
Cheng, A. F. and Ruderman, M. A. 1980, Particle acceleration and radio emission above pulsar polar caps, Astrophys. J., 235, 576–586.Google Scholar
Cheng, K. S., Ho, C., and Ruderman, M. 1986a, Energetic radiation from rapidly spinning pulsars: I. Outer magnetospheric gaps Astrophys. J., 300, 500–521.Google Scholar
Cheng, K. S., Ho, C., and Ruderman, M. 1986b, Energetic radiation from rapidly spinning pulsars: II. Vela and Crab, Astrophys. J., 300, 522–539.Google Scholar
Chevalier, R. A. 1984, The interaction of Crab-like supernova remnants with their surroundings, Astrophys. J., 280, 797–801.Google Scholar
Chew, G., Goldberger, M., and Low, F. 1954, Proc. Roy. Soc., A236, N1204.Google Scholar
Chian, A. C. L. 1979, Nonlinear travelling longitudinal waves in cold plasmas, Plasma Phys., 21, 509.Google Scholar
Chian, A. C. L. 1981, Relativistically strong coupled transverse-longitudinal waves in an electron-ion plasma, Phys. Rev., A24, 2773.Google Scholar
Chian, A. C. L. 1982, On the self-consistent solutions of puisar plasma waves, Astr. Astrophys., 112, 391.Google Scholar
Chian, A. C. L. 1989, Wavebreaking condition of space-charge waves in a relativistic electron beam, Phys. Rev., A39, 2561.Google Scholar
Chian, A. C. L. and Clemow, P. C. 1975, Nonlinear periodic waves in a cold plasma: A quantitative analysis, J. Plasma Phys., 14, 505.Google Scholar
Chian, A. C. L. and Kennel, K. F. 1983, Self-modulational formation of pulsar microstructures, Astrophys. Space Sci., 97, 8–18.Google Scholar
Chiu, H. Y. 1972, Pulsars—Rotating magnetic neutron stars, in The Physics of Pulsars, ed. Lenchek, A. M., (New York: Gordon and Breach), 135.Google Scholar
Chiu, H. Y. and Canuto, V. 1971, Theory of radiation mechanisms of pulsars. I, Astrophys. J., 163, 577–594.Google Scholar
Chiueh, T. 1989, Relativistic solitons and shocks in magnetized e∼ - e+ - p+ fluids, Phys. Rev. Lett., 63, 113.Google Scholar
Chugunov, Y. V. and Shaposhnikov, V. E. 1988, Curvature radiation of a radio maser in a pulsar magnetosphere, Astrophysics, 28, 98.Google Scholar
Clark, and Eardley, D. M. 1976, Evolution of close neutron star binaries, Astrophys. J., 215, 311–322.Google Scholar
Cocke, W. J. 1973, Stimulated linear acceleration radiation: A pulsar radio emission mechanism, Astrophys. J., 184, 291–300.Google Scholar
Cordes, J. M. 1975, Pulsar PSR 1919+21: Notches, drifting subpulses, microstructure, and other emission, Astrophys. J., 195, 193–202.Google Scholar
Cordes, J. M. 1976a, Correlation analyses of microstructure and noiselike intensity fluctuations from pulsar PSR 2016+28, Astrophys. J., 208, 944–954.Google Scholar
Cordes, J. M. 1976b, Pulsar radiation as polarized shot noise, Astrophys. J., 210, 780–791.Google Scholar
Cordes, J. M. 1978, Observational limits on the location of pulsar emission regions, Astrophys. J., 222, 1006–1011.Google Scholar
Cordes, J. M. 1979, Coherent radio emission from pulsars, Space Sei. Rev., 24, 567.Google Scholar
Cordes, J. M. 1981, Radio observational constraints on pulsar emission mechanisms, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 115–131.Google Scholar
Cordes, J. M. 1986, Space velocities of radio pulsars from interstellar scintillations, Astrophys. J., 311, 183–196.Google Scholar
Cordes, J. M. 1992, Phenomenologica] constraints on polarcap models, in The Magneto spheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 254–261.Google Scholar
Cordes, J. M. and Downs, G. S. 1985, JPL Pulsar timing observations: III. Pulsar rotation fluctuations, Astrophys. J. Supp. Series, 59, 343–382.Google Scholar
Cordes, J. M. and Hankins, T. H. 1977, Pulsar polarization fluctuations at 430 MHz with microsecond time resolution, Astrophys. J., 218, 484–503.Google Scholar
Cordes, J. M. and Hankins, T. H. 1979, Frequency structure of micropulses from pulsar PSR 0950+08, Astrophys. J., 233, 981–986.Google Scholar
Cordes, J. M. and Helfand, D. J. 1980, Pulsar Timing III. Timing noise of 50 pulsars, Astrophys. J., 239, 640–650.Google Scholar
Cordes, J. M., Pidwerbetsky, A., and Lovelace, R. V. E. 1986, Refractive and diffractive scattering in the interstellar medium, Astrophys. J., 310, 737–767.Google Scholar
Cordes, J. M. and Stinebring, D. R. 1984, Multifrequency timing measurements on the millisecond pulsar PSR 1937+21, Astrophys. J., 277, L53–L56.Google Scholar
Cordes, J. M., Weisberg, J. M., and Boriakoff, V. 1983, An attempt to resolve pulsar magnetospheres using interstellar scintillations, Astrophys. J., 268, 370–380.Google Scholar
Cordes, J. M., Weisberg, J. M., and Hankins, T. H. 1990, Quasiperiodic microstructure in radio pulsar emissions, Astron. J., 100, 1882–1891.Google Scholar
Cordes, J. M. and Wolszczan, A. 1988, Interstellar interferometry, in Radio Wave Scattering in the Interstellar Medium, AIP Proc. No. 174, ed. Cordes, J. M., Rickett, B. J., and Backer, D. C., (New York: AIP), 212–216.Google Scholar
Cordes, J. M., Wolszczan, A., Dewey, R. J., Blaskiewicz, M., and Stinebring, D. R. 1990, Timing and scintillations of the millisecond pulsar 1937+214, Astrophys. J., 349, 245–261.Google Scholar
Córdova, F. A., Hjellming, R. M., Mason, K. D., and Middleditch, J. 1989, Soft x-ray emission from the radio pulsar PSR0656+14, Astrophys. J., 345, 451–463.Google Scholar
Coroniti, F. V. 1990, Magnetically stripped relativistic MHD winds: The Crab nebula revisited, Astrophys. J., 349, 538–545.Google Scholar
Coté, J. and Pylyser, E. H. P. 1989, On the birthrates of galactic low-mass binary radio pulsars and their possible progenitor systems, Astr. Astrophys., 218, 131.Google Scholar
Cox, J. L. Jr. 1979, Coherent radiation from pulsars, Astrophys. J., 229, 734–741.Google Scholar
Cox, J. L. Jr. 1980, Theory of Stellar Pulsation, (Princeton: Princeton University Press).Google Scholar
Craft, H. D. Jr. 1970, Radio observations of the pulse profiles and dispersion measures of twelve pulsars. PhD thesis, Cornell University.Google Scholar
Craft, H. D. Jr., Cornelia, J. M., and Drake, F. D. 1968, Submillisecond radio intensity variations in pulsars, Nature, 218, 1122.Google Scholar
da Costa, A. A. and Kahn, F. D. 1985, Pulsar electrodynamics: The back reaction of the motion of charged particles, Mon. Not. R. astr. Soc, 215, 701.Google Scholar
Damour, T. and Ruffini, R. 1974, Comptes Rendus, 279A, 971.Google Scholar
Daugherty, J. K. and Harding, A. K. 1982, Electromagnetic cascades in pulsars, Astrophys. J., 252, 337–347.Google Scholar
Daugherty, J. K. and Harding, A. K. 1986, Compton Scattering in strong magnetic fields, Astrophys. J., 309, 362–371.Google Scholar
Daugherty, J. K. and Harding, A. K. 1989, Comptonization of thermal photons by relativistic electron beams, Astrophys. J., 336, 861–874.Google Scholar
Davidson, K. and Fesen, R. A. 1985, Recent developments concerning the Crab nebula, Ann. Rev. Astr. Ap., 23, 119–146.Google Scholar
Davies, J. G., Lyne, A. G., Graham-Smith, F., Izvekova, V. A., Kuz'min, A. D., and Shitov, Y. P. 1984, The magnetic field structure of PSR 0809+74, Mon. Not. R. astr. Soc., 211, 57.CrossRefGoogle Scholar
Davies, J. G., Lyne, A. G., and Seiradakis, J. H. 1977, The galactic distribution of pulsars, Mon. Not. ft. astr. Soc, 179, 635–650.Google Scholar
Davis, L. and Goldstein, M. 1970, Magnetic-dipole alignment in pulsars, Astrophys. J.. 159, L81–L85.Google Scholar
de Jager, O. C. 1990. Preprint on AE Aqu.Google Scholar
de Kool, M. and van Paradijs, J. 1986, Neutron star spin evolution in wide low-mass x-ray binaries, Astr. Astrophys., 173, 279–283.Google Scholar
Deich, W. T. S., Cordes, J. M., Hankins, T. H., and Rankin, J. M. 1986, Null transition times, quantised drift modes, and no memory across nulls for PSR 1944 ± 17, Astrophys. J., 300, 540–550.Google Scholar
Deng, Z. G., Huang, J. H., and Xia, X. Y. 1987, The evolution of two types of pulsars, Ap. Sp. Sci., 129, 503.Google Scholar
Dermer, C. D. 1990, Compton scattering in strong magnetic fields and the continuum spectra of gamma ray bursts: Basic theory, Astrophys. J., 360, 197–214.Google Scholar
Deshpande, A. A. 1987. PhD thesis, Indian Institute of Technology, Bombay.Google Scholar
Deshpande, A. A. 1990. in preparation.Google Scholar
Deshpande, A. A., Shevgaonkar, R. K., and Sastry, C. V. 1989, Journal of IETE, 35, 342.Google Scholar
Deutsch, A. J. 1955, The electromagnetic field of an idealized star in rigid rotation in vacuuo, Ann. Astrophys., 18, 1.Google Scholar
Downs, G. S. 1979, Integrated pulse profiles and mean fluxes of 24 pulsars at 2.388 gigahertz, Astrophys. J. Supp. Series, 40, 365–369.Google Scholar
Downs, G. S. and Reichley, P. E. 1983, JPL pulsar timing observations. II. Geocentric arrival times., Astrophys. J. Supp. Series, 53, 169–240.Google Scholar
Drake, F. D. and Craft, H. D. 1968, Second periodic pulsations in pulsars, Nature, 220, 231–235.Google Scholar
Durdin, J. M., Large, M. I., Little, A. G., Manchester, R. N., Lyne, A. G., and Taylor, J. H. 1979, An unusual pulsar— PSR 0826-34, Mon. Not. R. astr. Soc, 186, 39P–41P.Google Scholar
Egorenko, V. D., Lominadze, D. G., and Mamradze, P. G. 1983, Beam instability of the plasma in pulsar magnetospheres, Astrophysics, 19, 426.Google Scholar
Eidman, V. Y. 1971, On the radiation of electromagnetic waves by relativistic clusters of charged particles, Astrofizica, 7, 135.Google Scholar
Elitzur, M. 1982, Physical characteristics of astronomical masers, Reviews of Modern Physics, 54, 1225.Google Scholar
Ellison, D. E., Jones, F. C., and Reynolds, S. P. 1990, First-order Fermi particle acceleration by relativistic shocks, Astrophys. J., 360(2), 702–714.Google Scholar
Elsasser, K. and Kirk, J. 1976, Pulsar signals from relativistic electron beams, Astr. Astrophys., 52, 449.Google Scholar
Emmering, R. T. and Chevalier, R. A. 1987, Shocked relativistic magnetohydrodynamic flows with application to pulsar winds, Astrophys. J., 321, 334–348.Google Scholar
Emmering, R. T. and Chevalier, R. A. 1989, The intrinsic luminosity and initial period of pulsars, Astrophys. J., 345, 931–938.Google Scholar
Epstein, R. I. 1985, Feeding a gamma-ray burster, Astrophys. J., 291, 822–833.Google Scholar
Erickson, W. C. and Mahoney, M. J. 1985, The radio continuum spectrum of PSR 1937+214, Astrophys. J., 299, L29–L31.Google Scholar
Erickson, W. C., Mahoney, M. J., Becker, R. H., and Helfand, D. J. 1987, VLA observations of the fast pulsar candidate in M28, Astrophys. J., 314, L45–L47.Google Scholar
Ertl, T. 1988, Selbstkonsistente Behandlung von Pulsarmagnetosphären. PhD thesis, Universitä;t Tü;bingen.Google Scholar
Ertl, T., Herold, H., Finkbeiner, B., and Ruder, H. 1987, Self-consistent modelling of pulsar magnetospheres, Mitt. Astron. Ges., 70, 372.Google Scholar
Esposito, L. W. and Harrison, E. R. 1975, Properties of the Hulse-Taylor binary pulsar system, Astrophys. J., 196, L1–L2.Google Scholar
Ewing, M. S., Batchelor, R. A., Friedfeld, R. D., Price, R. M., and Staelin, D. H. 1970, Observations of pulsar spectra, Astrophys. J., 162, L169–L172.Google Scholar
Fawley, W. M. 1978, Particle acceleration, gamma-ray emission and sparking in pulsars. PhD thesis, University of California at Berkeley.Google Scholar
Fawley, W. M., Arons, J., and Scharlemann, E. T. 1977, Potential drops above pulsar polar caps: Acceleration of nonneutral beams form the stellar surface, Astrophys. J., 217, 227–243.Google Scholar
Ferguson, D. C. 1981, Pulse emission from the light cylinder, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 141–152.Google Scholar
Ferguson, D. C. and Boriakoff, V. 1980, Short time scale integrated pulse shape variations in PSR 0611+22, Astrophys. J., 239, 310–315.Google Scholar
Ferguson, D. C., Boriakoff, V., Weisberg, J. M., Backus, P. R., and Cordes, J. M. 1981, Discovery of mode switching in PSR 1926+18, Astr. Astrophys., 94, L6–L8.Google Scholar
Ferguson, D. C. and Seiradakis, J. H. 1978, A detailed, high time resolution study of high frequency radio emission from PSR 1133+16, Astr. Astrophys., 64, 27.Google Scholar
Fesen, C. 1990. personal communication.Google Scholar
Filippenko, A. V. and Radhakrishnan, V. 1982, Pulsar nulling and drifting subpulse phase memory, Astrophys. J., 263, 828–834.Google Scholar
Finkbeiner, B., Herold, H., Ertl, T., and Ruder, H. 1989, Effects of radiation damping on particle motion in pulsar vacuum fields, Astr. Astrophys., 225, 479.Google Scholar
Fisher, R. J. 12 June 1982. NRAO Internal Memo.Google Scholar
Fitzpatrick, R. 1988. PhD thesis, University of Sussex.Google Scholar
Fitzpatrick, R. and Mestel, L. 1988a, Pulsar electrodynamics- I, Mon. Not. R. astr. Soc., 232, 277–302.Google Scholar
Fitzpatrick, R. and Mestel, L. 1988b, Pulsar electrodynamics- II, Mon. Not. R. astr. Soc., 232, 303–321.Google Scholar
Flanagan, C. 1989. IAU circular 4695.Google Scholar
Flowers, E. and Itoh, N. 1976, Transport properties of dense matter, Astrophys. J., 206-242, 218.Google Scholar
Flowers, E. and Ruderman, M. A. 1977, Evolution of pulsar magnetic fields, Astrophys. J., 215, 302–310.Google Scholar
Flowers, E. G., Lee, J. F., Ruderman, M. A., Sutherland, P. G., Hillebrandt, W., and Müller, W. 1977, Variational calculation of ground-state energy of condensed matter: Iron atoms in strong magnetic fields, Astrophys. J., 215, 291–301.Google Scholar
Foster, R. S. and Backer, D. C. 1990, Constructing a pulsar timing array, Astrophys. J., 361, 300–308.Google Scholar
Foster, R. S. and Cordes, J. M. 1990, Interstellar propagation effects and the precision of pulsar timing, Astrophys. J., 364, 123–135.Google Scholar
Fowler, L. A., Wright, G. A. E., and Morris, D. 1981, Unusual properties of the pulsar PSR 1822—09, Astr. Astrophys., 93, 54–61.Google Scholar
Fracassini, M., Pasinetti, L. E., and Rafaelli, G. 1986, Discriminant analysis of pulsar groups in the diagram P vs. Ṗ, in Proc. of the Joint Varenna-Abastumani School and Workshop on Plasma Astrophys., ESA SP-285, (Noordwijk: ESA Publications Division), 315.Google Scholar
Fruchter, A. S. et al.. 1990, The eclipsing millisecond pulsar PSR 1957+20, Astrophys. J., 351, 642–650.Google Scholar
Fruchter, A. S., Stinebring, D. R., and Taylor, J. H. 1988, A millisecond pulsar in an eclipsing binary, Nature, 333, 237–239.Google Scholar
Gallant, Y. A., Hoshino, M., Langdon, A. B., Arons, J., and Max, C. E. 1990, Structure of relativistic magnetosonic shocks in electron-positron plasmas, Astrophys. J., to be submitted.Google Scholar
Gedalin, M. E. and Machabeli, G. Z. 1983, Oblique waves propagating in a relativistic electron-positron plasma, Astrophysics, 19, 91.Google Scholar
Ghosh, P. and Lamb, F. K. 1979, Accretion by rotating magnetic neutron stars: III. accretion torques and period changes in pulsating x-ray sources, Astrophys. J., 234, 296–316.Google Scholar
Gil, J. A. 1981, The frequency dependence of micropulse separation, Astr. Astrophys., 104, 69–71.Google Scholar
Gil, J. A. 1983, Lorentz factor of particles emitting in pulsars, Astr. Astrophys., 123, 7.Google Scholar
Gil, J. A. 1984, A new aspect of the hollow-cone model of pulsar emission, Astr. Astrophys., 131, 67–71.Google Scholar
Gil, J. A. 1985, Interpulse beams and profile components, Astrophys. J., 299, 154–160.Google Scholar
Gil, J. A. 1986, Triplicity of pulsar profiles and orthogonal polarisation modes, Astrophys. J., 309, 609–618.Google Scholar
Gil, J. A. 1992, Curvature radiation and polarized emission from PSR 2303+30, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 395–400.Google Scholar
Gil, J. A., Hankins, T. H., Stinebring, D. R., and Snakowski, J. K. 1992, The geometry of PSR 0525+21, Astrophys. J., submitted.Google Scholar
Gil, J. A. and Snakowski, J. K. 1990a, Curvature radiation and the core emission of pulsars, Astr. Astrophys., 234, 237–242.Google Scholar
Gil, J. A. and Snakowski, J. K. 1990b, Pulsar emission as curvature—generated polarized shot noise, Astr. Astrophys., 234, 269–272.Google Scholar
Ginzburg, V. L. 1982, Aatrofizica kosmicheskikh luchei, (Moscow: Nauka Press).Google Scholar
Ginzburg, V. L. and Zheleznyakov, V. V. 1975, On the pulsar emission mechanisms, Ann. Rev. Astr. Ap., 13, 511–535.Google Scholar
Glendenning, N. K. 1985, Neutron stars are giant hypernuclei?, Astrophys. J., 293, 470–493.Google Scholar
Gold, T. 1969, Rotating neutron stars and the nature of pulsars, Nature, 221, 25,Google Scholar
Gold, T. 1978, in Ninth Texas Symp. on Relativistic Astrophysics, ed. Ehlers, J., Perry, J. J., and Walker, M., volume 336, Ann. N. Y. Acad. Sci., 448.Google Scholar
Goldreich, P. 1970, Neutron star crust and the alignment of magnetic axes in pulsars, Astrophys. J., 160, Lll–L15.Google Scholar
Goldreich, P. and Julian, W. H. 1969, Pulsar electrodynamics, Astrophys. J., 157, 869–880.Google Scholar
Goldreich, P. and Julian, W. H. 1970, Stellar winds, Astrophys. J., 160, 971–977.Google Scholar
Goldreich, P. and Keeley, D. A. 1971, Coherent synchrotron radiation, Astrophys. J., 170, 463–477.Google Scholar
Goldstein, S. J. and James, J. T. 1969, Accurate dispersions for thirteen pulsars, Astrophys. J., 158, L179–L182.Google Scholar
Good, M. L. and Ng, K. K. 1970, Electromagnetic torques, secular alignment and spin-down of neutron stars, Astrophys. Lett., 299, 86.Google Scholar
Gould, D. M. and Lyne, A. G. 1990, in press.Google Scholar
Gower, J. F. R. and Argyle, E. 1972, Detection of strong interpuises from NP0532, Astrophys. J., 171, L23–L26.Google Scholar
Grassberger, P. and Procaccia, I. 1983a, Physica, 9D, 189.Google Scholar
Grassberger, P. and Procaccia, I. 1983b, Characterization of strange attractors, Phys. Rev. Lett., 50, 346.Google Scholar
Gross, M. and Haroche, S. 1982, Superradiance: An essay on theory of collective spontaneous emission, Phys. Rep., 93, 301.Google Scholar
Groth, E. J. 1975, Timing of the Crab pulsar III. The slowing down and the nature of the random process, Astrophys. J. Supp. Series, 29, 453–465.Google Scholar
Gunn, J. E. and Ostriker, J. P. 1970, On the nature of pulsars: III. Analysis of observations., Astrophys. J., 160, 979–1002.Google Scholar
Gunn, J. E. and Ostriker, J. P. 1971, On the motion and radiation of charged particles in strong electromagnetic waves: I. Motion in plane and spherical waves, Astrophys. J., 165, 523–541.Google Scholar
Gurevich, A. V. and Istomin, Y. N. 1985, Production of an electron-positron plasma in a pulsar magnetosphere, Soviet Phys. JETP, 62, 1–11.Google Scholar
Gurevich, A. V. and Levin, B. Y. 1950, Astron. Zh., 27, 273.Google Scholar
Guseiˇnov, O. H. and Yusifov, I. M. 1985a, Astron. Zh., 62, 240.Google Scholar
Guseiˇnov, O. H. and Yusifov, I. M. 1985b, Pulsar beam orientation, Sov. Astron., 29, 136–143.Google Scholar
Guseiˇnov, O. H. and Yusifov, I. M. 1991, On the shape of the pulsar emission pattern, Astron. Zh., 68, 529–537.Google Scholar
Haensel, P., Kutschera, M., and Prószyński, M. 1981, Uncertainty in the saturation density of nuclear matter and neutron star models, Astr. Astrophys., 102, 299–302.Google Scholar
Haensel, P. and Prószyński, M. 1982, Pion concentration in cold dense matter and neutron stars, Astrophys. J., 258, 306–320.Google Scholar
Haensel, P., Zdunik, J. L., and Schaeffer, R. 1986, Strange quark stars, Astr. Astrophys., 160, 121–128.Google Scholar
Hamilton, P. A., Hall, P. J., and Costa, M. E. 1985, Changing parameters along the path to the Vela pulsar, Mon. Not. R. aatr. Soc., 214, 5P–8P.Google Scholar
Hamilton, P. A., King, E. A., McConnell, D., and McCulloch, P. M. 1989. IAU circular 4708.Google Scholar
Hamilton, P. A., McCulloch, P. M., Abies, J. G., and Komesaroff, M. M. 1977a, Polarization characteristics of southern pulsars - I. 400-MHz observations, Mon. Not. R. aatr. Soc, 180, 1–18.Google Scholar
Hamilton, P. A., McCulloch, P. M., Manchester, R. N., Abies, J. G., and Komesaroff, M. M. 1977b, Nature, 265, 224.Google Scholar
Hankins, T. H. 1971, Microsecond intensity variation in the radio emission from CP0950, Astrophys. J., 169, 487–494.Google Scholar
Hankins, T. H. 1972, Short-time scale structure in two pulsars, Astrophys. J., 177, L11–L15.Google Scholar
Hankins, T. H. 1990. private communication.Google Scholar
Hankins, T. H. and Boriakoff, V. 1978, Submicrosecond time resolution observations of PSR 0950+08, Nature, 276, 45–47.Google Scholar
Hankins, T. H. and Boriakoff, V. 1981, Microstructure in the pulsar PSR 0950+08, Astrophys. J., 249, 238–240.Google Scholar
Hankins, T. H. and Cordes, J. M. 1981, Interpulse emission from pulsar 0950+08: How many poles?, Astrophys. J., 249, 241–253.Google Scholar
Hankins, T. H. and Fowler, L. A. 1982, Wide emission shoulders of radio pulsar profiles, Bull. American Astron. Soc., 14, 968.Google Scholar
Hankins, T. H. and Rickett, B. J. 1986, Frequency dependence of pulsar profiles, Astrophys. J., 311, 684–693.Google Scholar
Hankins, T. H. and Wolszczan, A. 1987, The drifting subpulse phenomenon observed in three pulsars with triple profiles, Astrophys. J., 318, 410–420.Google Scholar
Hardee, P. E. and Morrison, P. 1979, Plasma collective effects and pulsar emission models, Astrophys. J., 227, 252–265.Google Scholar
Hardee, P. E. and Rose, W. K. 1976, A mechanism for the production of pulsar radio radiation, Astrophys. J., 210, 533–538.Google Scholar
Hardee, P. E. and Rose, W. K. 1978, Wave production in an ultrarelativistic electron-positron plasma, Astrophys. J., 219, 274–287.Google Scholar
Harding, A. K., Shinbrot, T., and Cordes, J. M. 1989, A chaotic attractor in the timing noise from the Vela pulsar, Bull. American Astron. Soc., 21, 1205.Google Scholar
Harnden, F. R. Jr., Grant, P. D., Seward, F. D., and Kahn, S. M. 1985, EINSTEIN observations of Vela X and Vela pulsar, Astrophys. J., 299, 828–838.Google Scholar
Harnden, F. R. Jr. and Seward, F. D. 1984, EINSTEIN observations of the Crab nebula pulsar, Astrophys. J., 283, 279–285.Google Scholar
Hartle, J. B. 1978, Phys. Rep., 46, 201.Google Scholar
Harwit, M. and Salpeter, E. E. 1973, Radiation from comets near neutron stars, Astrophys. J., 186, L37–L39.Google Scholar
Hasegawa, A. 1975, Plasma Instabilities and Nonlinear Effects, (Berlin: Springer-Verlag).Google Scholar
He, Z. X., Qing, C. R., Qiao, G. J., and Wang, Y. R. 1990, An induced collapse model of SN1987A, preprint.Google Scholar
Heiles, C., Campbell, D. B., and Rankin, J. M. 1970, Pulsar NP 0532: Properties and systematic polarization of individual strong pulses at 430 MHz, Nature, 226, 529–531.Google Scholar
Heiles, C. E., Kulkarm, S. R., Stevens, M. A., Backer, D. C., Goss, W. M., and Davis, M. M. 1983, Distance to the 1.5 ms pulsar and other 4c21.53 objects, Astrophys. J., 273, L75–L79.Google Scholar
Heiles, C. E. and Rankin, J. M. 1971, Frequency structure in individual strong pulses of NP 0532, Nature Phys. Set., 231, 97–99.Google Scholar
Helfand, D. J. 1983, X-rays from radio pulsars: The portable supernova remnants, in I AU Symp. 101, Supernova Remnants and their X-ray Emission, ed. Gorenstein, P. and Danziger, J., (Dordrecht: D. Reidel), 471.Google Scholar
Helfand, D. J. 1984, X-ray sychrotron nebulae and the origin of neutron stars, Adv. Space Res., 3, 29.Google Scholar
Helfand, D. J., Manchester, R. N., and Taylor, J. H. 1975, Observations of pulsar radio emission: III. Stability of integrated profiles., Astrophys. J., 198, 661–670.Google Scholar
Holfand, D. J. and Tademaru, E. 1977, Pulsar velocity observations:Correlations, interpretations and discussion, Astrophys. J., 216, 842–851.Google Scholar
Helfend, D. J., Taylor, J. H., Backus, P. R., and Cordes, J. M. 1980, Pulsar timing: I. Observations from 1970 to 1978, Astrophys. J., 237, 206–215.Google Scholar
Hernquist, L. and Applegate, J. H. 1984, Analytical models of neutron star envelopes, Astrophys. J., 287, 244–254.Google Scholar
Herold, H. 1979, Compton and Thompson scattering in strong magnetic fields, Phys. Rev., D 19, 2868.Google Scholar
Herold, H., Ertl, T., Finkbeiner, B., and Ruder, H. 1989, Self-consistent modelling of pulsar magnetospheres, in Timing Neutron Stars, ed. Ögelman, H. and Heuvel, E. P. J. van den, (Dordrecht: Kluwer), 723.Google Scholar
Herold, H., Ertl, T., and Ruder, H. 1985, Generation of relativistic particles in pulsar magnetospheres, Mitt. Astron. Ges., 63, 174.Google Scholar
Herold, H., Ertl, T., and Ruder, H. 1986, Towards a selfconsistent modelling of pulsar magnetospheres, in Proc. of the 8th EPS Conference on Computational Physics — Computing in Plasma Physics, volume 10D, Europhysics Conference Abstracts, 3.Google Scholar
Hewish, A. 1981, Introductory review, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 1–6.Google Scholar
Heygi, D., Novick, R., and Thaddeus, P. 1971, A search for variations in the intensity of the optical pulses from NP 0532, in The Crab Nebula, IAU Symp. No. 46, ed. Davies, R. D. and Smith, F. G., (Dordrecht: D. Reidel).Google Scholar
Hinata, S. 1976a, Level of electrostatic excitation associated with the relativistic beam-plasma system and pulsar radiation, Astrophys. Space Sci., 44, 389.Google Scholar
Hinata, S. 1976b, Relativistic plasma turbulence and its application to pulsar phenomena, Astrophys. J., 206, 282–294.Google Scholar
Hinata, S. 1976c, Stability of a beam-plasma system against the excitation of the longitudinal mode around pulsars, Astrophys. J., 203, 223–225.Google Scholar
Holloway, N. J. 1973, p-n junctions in pulsar magnetospheres, Nature, 246, 6.Google Scholar
Holloway, N. J. 1977, Angular momentum and energy loss from pulsars, Mon. Not. R. astr. Soc., 181, 9P.Google Scholar
Horn, S. and Kundt, W. 1989, Magnetically tilted accretion disks, Astrophys. Space Sci., 158, 205–221.Google Scholar
Hoshino, M. and Arons, J. 1990, Differential heating and acceleration of positrons by sychrotron maser instabilities, Phys. Fluids, submitted.Google Scholar
Hoshino, M., Arons, J., Langdon, A. B., Gallant, Y. A., and Max, C. E. 1990, Differential heating and acceleration of positrons in electron-positron-proton relativistic magnetosonic shocks, Astrophys. J., submitted.Google Scholar
Huguenin, G. R., Manchester, R. N., and Taylor, J. H. 1971, Properties of pulsars, Astrophys. J., 169, 97.Google Scholar
Huguenin, G. R., Taylor, J. H., and Troland, T. H. 1970, The radio emission from pulsar MP 0031—07, Astrophys. J., 162, 727–735.Google Scholar
Hunt, G. C. 1971, The rate of change of period of the pulsars, Mon. Not. R. astr. Soc., 153, 119–131.Google Scholar
Imre, K. 1962, Oscillations in a relativistic plasma, Phys. Fluids, 5(4), 459–466.Google Scholar
Isobe, T., Feigelson, E. D., and Nelson, P. I. 1986, Statistical methods for astronomical data with upper limits: II. Correlation and regression, Astrophys. J., 306, 490–507.Google Scholar
Istomin, Y. N. 1988, Nonlinear interaction of waves in an inhomogeneous plasma, Soviet Phys. JETP, 67, 1380.Google Scholar
Izvekova, V. A., Kuz'min, A. D., Malofeev, V. M., Jessner, A., Sieber, W., and Wielebinski, R. 1990, New evidence of multipole magnetic field structure of pulsars, Astr. Astrophys. in preparation.Google Scholar
Izvekova, V. A., Kuz'min, A. D., Malofeev, V. M., and Shitov, Y. P. 1979, Radio flux density and pulse profiles of pulsars at 102.5 and 61 MHz, Sov. Astron., 23, 179–188.Google Scholar
Izvekova, V. A., Kuz'min, A. D., Malofeev, V. M., and Shitov, Y. P. 1981, Radio spectra of pulsars I. Observations of flux densities at meter wavelengths and analysis of the spectra, Astrophys. Space Sci., 78, 45–72.Google Scholar
Izvekova, V. A., Kuz'min, A. D., Malofeev, V. M., and Shitov, Y. P. 1989, Frequency variations of the form and time alignment of the pulsars mean profiles, J. Lebedev Physical Inst., 199, 13.Google Scholar
Izvekova, V. A., Kuz'min, A. D., and Shitov, Y. P. 1982, Detection of the regular “abnormally” directed drift of subpulses of the pulsar PSR 0320+39, Sev. Astron., 26, 324–327.Google Scholar
Izvekova, V. A., Malov, I. F., and Malofeev, V. M. 1977, On the applicability of the hollow-cone beam model to pulsars, Pis'ma Astron. Zh., 3, 442–445.(in Russian).Google Scholar
Jackson, E. A. 1976, A new pulsar atmospheric model: Aligned magnetic and rotational axes, Astrophys. J., 206, 831.Google Scholar
Jackson, E. A. 1980, Finite force-free pulsar atmosphere models, Astrophys. J., 237, 198–205.Google Scholar
Jackson, J. D. 1962, Classical Electrodynamics, (New York: Wiley).Google Scholar
Javakhishvili, J. I. and Tsintsadze, N. L. 1973, Transport phenomena in a completely ionized ultra relativistic plasma, Soviet Phys. JETP, 37, 666–671.Google Scholar
Jones, P. B. 1977, Pulsar magnetic alignment: a classification of pulsars, Mon. Not. R. astr. Soc., 178, 87P–91P.Google Scholar
Jones, P. B. 1978, Particle acceleration at the magnetic poles of a neutron star, Mon. Not. R. astr. Soc., 184, 807–823.Google Scholar
Jones, P. B. 1979, Pair production on the pulsar magnetosphere, Astrophys. J., 228, 536–540.Google Scholar
Jones, P. B. 1980a, The elliptical cross section and linear polarization of pulsar radio beams, Astrophys. J., 236, 661–663.Google Scholar
Jones, P. B. 1980b, Source of coherent radio emission in pulsars, Astrophys. J., 237, 590.Google Scholar
Jones, P. B. 1981, A model of the normal and null states of pulsars, Mon. Not. R. astr. Soc., 197, 1103–1124.Google Scholar
Jones, P. B. 1986, Density functional calculations of the cohesive energy of condensed matter in very strong magnetic fields, Mon. Not. R. ostr. Soc, 218, 477.Google Scholar
Jones, P. B. 1987, Neutron star magnetic field decay: Flux expulsion from the superconducting interior, Mon. Not. R. astr. Soc., 228, 513.Google Scholar
Jones, P. B. 1988, Neutron star magnetic field decay: Hall drift and ohmic diffusion, Mon. Not. R. astr. Soc., 233, 875–885.Google Scholar
Julian, W. H. 1973, Pulsar electrodynamics II, Astrophys. J., 183, 967.Google Scholar
Kadomtzev, V. V. 1988, Kollektivnye yavleniya v plasme, (Moscow: Nauka Press).Google Scholar
Kahn, F. D. and Lerche, I. 1965, Radiation from cosmic ray air showers, Proc. Roy. Soc. bond A, 289, 206.Google Scholar
Kaplan, S. A. 1968, On the theory of coherent synchrotron radiation from cosmic radio sources, Astrophysics, 2, 221.Google Scholar
Kaplan, S. A. and Tsytovich, V. N. 1973, Plasma Astrophysics, (London: Pergamon Press).Google Scholar
Kapoor, R. C. and Datta, B. 1985, Fast pulsars? Effects of spacetime curvature and rotation on the pulse characteristics, Astrophys. J., 297, 413.Google Scholar
Kardeshev, N. S. et al.. 1978, Pulsar observations with a time resolution of 10 microseconds at 102.5MHz, Sov. Astron., 22, 583–587.Google Scholar
Kardeshev, N. S. et al.. 1982, PSR 1133+16: Determination of the dispersion measure and the location of the emitting regions, Astr. Astrophys., 109, 340–343.Google Scholar
Kardeshev, N. S. et al.. 1986, Simultaneous single-pulse observations of radio pulsars over a broad frequency range ii. Correlation between intensities of single pulses at 102.5 and 1700MHz, Astr. Astrophys., 163, 114.Google Scholar
Karpman, V. I. and Maslov, E. M. 1977, Perturbation theory for solitons, Soviet Phys. JETP, 46, 281.Google Scholar
Kawasura, K. and Suzuki, I. 1977, A model of the radio emission mechanism in pulsars, Astrophys. J., 217, 832.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., and Melikidze, G. I. 1987a, Influence of inhomogeneity of the magnetic field on excitation of longitudinal waves in pulsar magnetospheres, Astrophysics, 25, 425.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., and Melikidze, G. I. 1987b, Radio emission of a ‘typical’ pulsar, Aust. J. Phys., 40, 755–766.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., and Melikidze, G. I. 1989, in Proc. of the Joint Varenna-Abastumani School and Workshop on Plasma Astrophys., ESA SP-285, volume 1, (Noordwijk: ESA Publications Division), 277.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., and Melikidze, G. I. 1992a, A mechanism of circular polarization in pulsar radiation, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars. IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 374–375.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., and Melikidze, G. I. 1992b, A model for the drifting subpulse phenomenon, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 297–299.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., and Melikidze, G. I. 1992c, On a possible mechanism of pulsar radiation, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 233–236.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., Melikidze, G. I., and Usov, V. V. 1988, On the nature of a ‘typical’ pulsar radio emission, in Proc. of the Joint Varenna-Abastumani School and Workshop on Plasma Astrophys., ESA SP-285, volum. 1, 271.Google Scholar
Kennel, C. F. and Coroniti, F. V. 1984a, Confinement of the Crab pulsar's wind by its supernova remnant, Astrophys. J., 283, 694.Google Scholar
Kennel, C. F. and Coroniti, F. V. 1984b, Magnetohydrodynamic model of Crab nebula radiation, Astrophys. J., 283, 710.Google Scholar
Kennel, C. F., Fugimura, F., and Okamoto, I. 1983, Relativistic magnetohydrodynamic winds of finite temperature, Geophys. and Astrophys. Fluid Dyn., 26, 147.Google Scholar
Kennel, C. F. and Pellat, R. 1976, Relativistic noli near waves in a magnetic field, J. Plasma Phys., 15, 335.Google Scholar
Kirk, J. G. 1980, Coherent curvature radiation, Astr. Astrophys., 82, 262.Google Scholar
Kluźniak, W., Ruderman, M., Shaham, J., and Tavani, M. 1988, Nature and evolution of the eclipsing millisecond binary pulsar PSR 1957+20, Nature, 334, 225–227.Google Scholar
Knight, F. K., Matteson, J. L., Peterson, L. E., and Rothschild, R. E. 1982, X-ray and gamma-ray upper limits for pulsed emission from radio pulsars, Astrophys. J., 260, 553.Google Scholar
Kocharovskii, V. V. and Kocharovskii, V. V. 1990, Phenomenological quantum electrodynamics of active media and superradiance, in Nonlinear waves, ed. Gaponov-Grehkov, A. V. and Rabinovich, M. I., (Berlin: Springer-Verlag).Google Scholar
Kolosov, D. E., Lipunov, V. M., Postnov, K. A., and Prokhorov, M. E. 1989, Astr. Astrophys.. 215, L21.Google Scholar
Komesaroff, M. M. 1970, Possible mechanism for the pulsar radio emission, Nature, 225, 612.Google Scholar
Kössl, D., Wolff, R. G., Miller, E., and Hillerbrandt, W. 1988, Density functional calculations in strong magnetic fields: The ground state properties of atoms, Astr. Astrophys., 205, 347–353.Google Scholar
Kovalev, Y. A. 1979, A possible radio emission mechanism for pulsars, Astrophys. Space Sci., 63, 3–17.Google Scholar
Kovalev, Y. A. 1980, Crab pulsar: Magnetized cracks in the crust as a key to mechanisms of the matter flow, radio and high-frequency emission, Astrophys. Space Sci., 67, 387.Google Scholar
Koyama, K. 1988, X-ray observations with the Ginga satellite, Comm. Astrophys., 12, 287.Google Scholar
Krauese-Pohlstorff, J. and Michel, F. C. 1985a, Electrosphere of an aligned magnetized neutron star, Mon. Not. R. astr. Soc., 213, 43P.Google Scholar
Krausse-Pohlstorff, J. and Michel, F. C. 1985b, Pulsar space charging, Astr. Astrophys., 144, 72.Google Scholar
Krishnamohan, S. and Downs, G. S. 1983, Intensity dependence of the pulse profile and polarization of the Vela pulsar, Astrophys. J., 265, 372.Google Scholar
Krishnan, V. and Sivaram, C. 1983, Radio emission by parallel acceleration emission mechanism, Solar Phys., 84, 125.Google Scholar
Kroll, N. M. and McMullin, W. A. 1979, Stimulated linear acceleration bremsstrahlung, Astrophys. J., 231, 425.Google Scholar
Kulkarni, S. R. 1986, Optical identification of binary pulsars: Implications for magnetic field decay in neutron stars, Astrophys. J., 306, L85–L89.Google Scholar
Kulkarni, S. R. 1990, in Neutron stars and their birth events, NATO ASI C, ed. Kundt, W., volume 300, (Dordrecht: Kluwer), 59.Google Scholar
Kulkarni, S. R. and Hester, J. J. 1988, Discovery of a nebula around PSR 1957+20, Nature, 335, 801–803.Google Scholar
Kulkarni, S. R. and Narayan, R. 1988, Birthrates of lowmass binary pulsars and low-mass X-ray binaries, Astrophys. J., 335, 755–768.Google Scholar
Kundt, W. 1981, Do neutron star magnetic fields decay?, Astr. Astrophys., 98, 207–210.Google Scholar
Kundt, W. 1985, What do we know about pulsars?, Bull. Astron. Soc. India, 13, 12–52.Google Scholar
Kundt, W. 1988, Do pulsar magnetic fields decay?, Comm. Astrophys., 12, 113.Google Scholar
Kundt, W. 1990a, Known and expected sources of low-frequency radiation, in Low-Frequency Astrophysics from Space, Lecture Notes in Physics, ed. Weiler, K. and Kassim, N., (New York: Springer-Verlag Lecture Notes in Physics Series), 239–251.Google Scholar
Kundt, W. 1990b, Observed neutron star properties, in Neutron Stars and Their Birth Events, ed. Kundt, W., volume 300, (Dordrecht: Kluwer Academic Publishers), 1–21.Google Scholar
Kundt, W. and Krotscheck, E. 1980, The Crab nebula-a model, Astr. Astrophys., 83, 1–21.Google Scholar
Kundt, W., Özel, M., and Ercan, E. N. 1987, Astr. Astrophys., 177, 163.Google Scholar
Kuo-Petravic, L. G., Petravic, M., and Roberts, R. W. 1974, Self-consistent solution for an axisymmetric pulsar model, Phys. Rev. Lett., 32, 1019.Google Scholar
Kuz'min, A. D. 1985a. Preprint No. 210 (in Russian). Technical report, Lebedev Physical Institute, USSR Academy of Sciences, Moscow.Google Scholar
Kuz'min, A. D. 1986, Frequency dependence of the dispersion measure and the extra dispersion time delay of the pulses for radio pulsars, Sov. Astron. Lett, 12, 778.Google Scholar
Kuz'min, A. D. 1989a, Influence of the scattering in interstellar medium on observed profile of the pulsars, FIAN Transactions, 199, 147.Google Scholar
Kuz'min, A. D., Alekseev, Y. A., Lapaev, K. A., Losovsky, B. Y., and Salnikov, A. A. 1990, Observations of the millisecond pulsar PSR 1855+09 at 102 MHz, Sov. Astron. Lett, 16, 208.Google Scholar
Kuz'min, A. D. and Dagkesamanskaya, I. M. 1983, Evaluations of the angle of magnetic axis and spin axis of 308 pulsars, Sov. Astron. Lett, 9, 80.Google Scholar
Kuz'min, A. D., Dagkesamanskaya, I. M., and Pugachev, V. D. 1984, The evolving orientation of the magnetic axis of pulsar?, Sov. Astron. Lett, 10, 357.Google Scholar
Kuz'min, A. D., Izvekova, V. A., Malofeev, V. M., and Shitov, Y. P. 1988, The scattering of pulse radioemission at 102 MHz. The difference from the dependence, Pis'ma Astron. Zh., 14, 140–144.Google Scholar
Kuz'min, A. D., Malofeev, V. M., Izvekova, V. A., Sieber, W., and Wielebinski, R. 1986, A comparision of highfrequency and low-frequency characteristics of pulsars, Astr. Astrophys., 161, 183–194.Google Scholar
Kuz'min, O. A. 1985b, Periodic microstructure in the pulses of PSR 1133+16 from synchronous observations at three meter wavelengths, Sov. Astron., 29, 133–136.Google Scholar
Kuz'min, O. A. 1989b. PhD thesis.Google Scholar
Kuz'min, O. A. 1992, Resolution of the PSR 1919+21 magnetosphere emitting region, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 288–290.Google Scholar
Lakhina, G. S. and Buti, B. 1981, Generation of a DC field by nonlinear electromagnetic waves in relativistic plasmas, Astrophys. Space Sci., 79, 25.Google Scholar
Landau, L. D. and Lifshitz, E. M. 1962, Teorya polya, (Moscow: Nauka Press).Google Scholar
Landau, L. D. and Lifshitz, E. M. 1967, Field Theory (in Russian), (Moscow: Nauka Press).Google Scholar
Landau, L. D. and Lifshitz, E. M. 1973, Electrodynamika sploshnykh sred, (Moscow: Nauka Press).Google Scholar
Landau, L. D. and Lifshitz, E. M. 1975, The Classical Theory of Fields, (Oxford: Pergamon Press).Google Scholar
Landau, L. D. and Lifshitz, E. M. 1982, Teoriya polya, (Moscow: Nauka Press).Google Scholar
Landau, L. D. and Lifshitz, E. M. 1986, Hydrodynamics (in Russian), (Moscow: Nauka Press).Google Scholar
Langdon, A. B., Arons, J., and Max, C. E. 1988, Structure of relativistic magnetosonic shocks in electron-positron plasmas, Phys. Rev. Lett., 61, 779.Google Scholar
Langer, S. 1981, Collisional excitation of electron Landau levels in strong magnetic fields, Phys. Rev., D 23, 328.Google Scholar
Larroche, O. and Pellat, R. 1987, Curvature instability of relativistic particle beams, Phys. Rev. Lett, 59, 1104.Google Scholar
Larroche, O. and Pesme, D. 1990, The source-driven dissipât ive nonlinear Schrödinger model of resonance absorption, Physica B, 2, 1751–1767.Google Scholar
Lattimer, J. M. and Schramm, D. N. 1979, The tidal disruption of neutron stars by black holes in close binaries, Astrophys. J., 210, 549–567.Google Scholar
Leboeuf, J. N., Ashour-Abdalla, M., Tajima, T., Kennel, C. F., Coroniti, F. V., and Dawson, J. M. 1982, Ultrarelativistic waves in overdense electron-positron plasma, Phys. Rev., A25, 1023.Google Scholar
Lerche, I. 1968, Enhanced bremsstrahlung from supraluminous, and subluminous, waves in an isotropic, homogeneous plasma, Phys. Fluids, 11, 2459.Google Scholar
Lindblom, L. 1984, Limits on the gravitational redshift from neutron staTS, Astrophys. J., 278, 364–368.Google Scholar
Linscott, I. R. and Hankins, T. H. 1981, Detection of the Crab giant pulses at high frequencies, Bull. American Astron. Soc., 12, 820.Google Scholar
Litvak, A. G. and Sergeev, A. M. 1978, One-dimensional collapse of plasma waves, Soviet Phys. JETP Letters, 27, 517.Google Scholar
Lochner, J. C., Swank, J. H., and Szymkowiak, A. E. 1989, A search for a dynamical at tract or in Cygnus X-l, Astrophys. J., 337, 823.Google Scholar
Lominadze, J. G., Machabeli, G. Z., Melikidze, G.I., and Pataraya, A. D. 1986, Magnetospheric plasma of a pulsar, Sov. J. Plasma Phys., 12, 712.Google Scholar
Lominadze, J. G., Machabeli, G. Z., and Usov, V. V. 1983, Theory of NP 0532 pulsar radiation and the nature of the activity of the Crab nebula, Astrophys. Space Sci., 90, 19–43.Google Scholar
Lominadze, J. G., Mikhailovskii, A. B., and Sagdeev, R. Z. 1979, Langmuir turbulence of a relativistic plasma in a strong magnetic field, Soviet Phys. JETP, 50, 927.Google Scholar
Lominadze, J. G., Stenflo, L., Tsytovich, V. N., and Wilhelmsson, H. 1982, A new explanation of the high effective temperatures in pulsar radio emission, Physica Scripta, 26, 455.Google Scholar
Lowson, M. V. and Jupe, R. J. 1974, Wave forms for a supersonic rotor, J. Sound Vib., 37, 475.Google Scholar
Lozinskaya, T. A. 1986, Supernovae and Stellar Wind, (Moscow: Nauka Press).Google Scholar
Lyne, A. G. 1983. private communication.Google Scholar
Lyne, A. G. 1987, A massive glitch in an old pulsar, Nature, 326, 569–571.Google Scholar
Lyne, A. G., Anderson, B., and Salter, M. J. 1982, The proper motions of 26 pulsars, Mon. Not. R. astr. Soc., 201, 503–520.Google Scholar
Lyne, A. G. and Ashworth, M. 1983, The affect of nulls upon subpulse drift in PSRs 0809+74 and 0818-13, Mon. Not. R. astr. Soc., 204, 519–536.Google Scholar
Lyne, A. G., Biggs, J. D., Brinklow, A., Ashworth, M., and McKenna, J. 1988, Discovery of a binary millisecond pulsar in the globular cluster M4, Nature, 332, 45.Google Scholar
Lyne, A. G., Brinklow, A., Middleditch, J., Kulkarni, S. R., Backer, D. C, and Clifton, T. R. 1987, The discovery of a millisecond pulsar in the globular cluster M28, Nature, 328, 399–401.Google Scholar
Lyne, A. G. and Graham-Smith, F. 1990, Pulsar Astronomy, (Cambridge: Cambridge Univ. Press).Google Scholar
Lyne, A. G., Johnston, S., Manchester, R. N., Staveley-Smith, L., D'Amico, N., Lim, J., Fruchter, A. S., and Goes, W. M. 1990a. IAU circular 4974.Google Scholar
Lyne, A. G. and Large, M. I. 1976, Unpublished work.Google Scholar
Lyne, A. G. and Manchester, R. N. 1988, The shape of pulsar radio beams, Mon. Not. R. astr. Soc, 234, 477508.Google Scholar
Lyne, A. G. et al. 1990b, An eclipsing millisecond pulsar in the globular cluster Terza 5, Nature, 347, 650–652.Google Scholar
Lyne, A. G., Manchester, R. N., and Taylor, J. H. 1985, The galactic population of pulsars, Mon. Not. R. astr. Soc., 213, 613.Google Scholar
Lyne, A. G., Pritchard, R. S., and Smith, F. G. 1988, Crab patear timing 1982-1987, Mon. Not. R. astr. Soc., 233, 667.Google Scholar
Lyne, A. G., Ritchings, R. T., and Smith, F. G. 1975, The period derivatives of pulsars, Mon. Not. R. astr. Soc., 171, 579.Google Scholar
Lyne, A. G., Smith, F. G., and Graham, D. A. 1971, Characteristics of the radio pulses from the pulsars, Mon. Not. R. astr. Soc., 153, 337.Google Scholar
Lyubarskii, Y. E. 1990, Equilibrium of the return current sheet and structure of the pulsar magnetosphere, Sov. Astron. Lett., 16(1), 16–20.Google Scholar
Macdonald, D. A. and Thome, K. S. 1982, Black hole electrodynamics: An absolute-space/time-universal formulation, Mon. Not. R. astr. Soc., 198, 345.Google Scholar
Macdonald, G. J. F. and Ness, N. F. 1961, A study of free oscillations of the Earth, Journal of Geophys. Research, 66, 1865–1911.Google Scholar
Machabeli, G. Z. and Usov, V. V. 1979, Sov. Astron. Lett., 5, 445.Google Scholar
Malofeev, V. M. and Malov, I. F. 1980, Mean spectra for 39 pulsars, and the interpretation of their characteristic features, Sov. Astron., 24, 54.Google Scholar
Malone, R. C., Johnson, M. B., and Bethe, H. A. 1975, Neutron star models with realistic high-density equations of state, Astrophys. J., 199, 741–748.Google Scholar
Malov, I. F. 1983, Energies of electrons and angles between the axis of magnetic field and rotation axis in pulsars, Astrofizica, 19, 161.Google Scholar
Malov, I. F. 1985, On the two pulsar types, Sov. Astron., 29, 144–147.Google Scholar
Malov, I. F. 1986, On the angles between the axis of magnetic dipole and the axis of rotation of pulsars, Astrofizica, 24, 507.Google Scholar
Malov, I. F. 1987, Two type of pulsars, Aust. J. Phys., 40, 731.Google Scholar
Malov, I. F. 1989, Prospects of a search for x-rays from aligned radio pulsars, Sov. Astron. Lett., 15, 196.Google Scholar
Malov, I. F. 1990, Angle between the magnetic field and the rotation axis in pulsars, Sov. Astron., 34, 189.Google Scholar
Malov, I. F. 1991, The distribution of emitting regions in pulsars' magnetospheres, Pis'ma Astron. Zh., 17, 595.Google Scholar
Malov, I. F. and Malofeev, V. M. 1981, Radio spectra of pulsars II. The interpretation'., Astrophys. Space Sci., 78, 73–83.Google Scholar
Malov, I. F. and Malofeev, V. M. 1992, On the nature of the high-frequency cutoff in the radio spectra of pulsars, in The Magneto spheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 154–156.Google Scholar
Manchester, R. N. 1971, Observations of pulsar polarization at 410 and 1665 MHz, Astrophys. J. Supp. Series, 23, 283–322.Google Scholar
Manchester, R. N. 1974, Pulsar radiation mechanisms: What are the critical experiments?, Science, 186, 66.Google Scholar
Manchester, R. N. 1990. personal communication.Google Scholar
Manchester, R. N., Durdin, J. M., and Newton, L. M. 1985, A second measurement of a pulsar braking index, Nature, 313, 374.Google Scholar
Manchester, R. N., Hamilton, P. A., and McCulloch, P. M. 1980, Polarization characteristics of southern pulsars - III. 1612-MHz observations, Mon. Not. R. astr. Soc., 192, 153–177.Google Scholar
Manchester, R. N., Lyne, A. G., D'Amico, N., Johnston, S., Lim, J., and Kniffen, D. A. 1990, A millisecond pulsar in 47 Tucanae, Nature, 345, 598.Google Scholar
Manchester, R. N. et al.. 1978, Optical observations of Southern pulsars, Mon. Not. R. astr. Soc, 184, 159–170.Google Scholar
Manchester, R. N. and Peterson, B. A. 1989, A braking index for PSR 0540-69, Astrophys. J., 342, L23.Google Scholar
Manchester, R. N. and Taylor, J. H. 1977, Pulsars, (San Francisco: Freeman).Google Scholar
Manchester, R. N. and Taylor, J. H. 1981, Observed and derived parameters for 330 pulsars, Astron. J., 86, 1953–1973.Google Scholar
Manchester, R. N., Taylor, J. H., and Huguenin, G. R. 1973, Frequency dependence of pulsar polarization, Astrophys. J., 179, L7–L10.Google Scholar
Manchester, R. N., Taylor, J. H., and Huguenin, G. R. 1975, Observations of pulsar radio emission. II. Polarization of individual pulses, Astrophys. J., 196, 83–102.Google Scholar
Matese, J. J. and Whitmire, D. P. 1980, Implications of emission zone limits for the Ruderman-Sutherland pulsar model, Astrophys. J., 235, 587–591.Google Scholar
Max, C. E. 1973, Parametric instability of a relativistically strong electromagnetic wave, Phys. Fluids, 16, 1480.Google Scholar
McCray, R. 1966, Possibility of maser action in cosmic radio sources, Science, 154, 1320.Google Scholar
McCulloch, P. M., Hamilton, P. A., Ables, J. G., and Komesaroff, M. M. 1976, PSR 1055-52—A pulsar resembling the Crab nebula pulsar, Mon. Not. R. astr. Soc, 175, 71P–75P.Google Scholar
McCulloch, P. M., Hamilton, P. A., Manchester, R. N., and Abies, J. G. 1978, Polarization characteristics of southern pulsars - II. 640-MHz observations, Mon. Not. R. astr. Soc., 183, 645–676.Google Scholar
McCulloch, P. M., Hamilton, P. A., Royle, G. W. R., and Manchester, R. N. 1983, Daily observations of a large period jump of the Vela pulsar, Nature, 302, 319–321.Google Scholar
McCulloch, P. M., Klekociuk, A. R., Hamilton, P. A., and Royle, G. W. R. 1987, Daily observations of three period jumps of the Vela pulsar, Aust. J. Phys., 40, 725–730.Google Scholar
McDermott, P. N., Savedoff, M. P., Van Horn, H. M., Zweible, E. G., and Hansen, C. J. 1984, Electromagnetic damping of neutron star oscillations, Astrophys. J., 281, 746–750.CrossRefGoogle Scholar
McDermott, P. N., Van Horn, H. M., and Hansen, C. J. 1988, Nonradial oscillations of neutron stars, Astrophys. J., 325, 725–748.Google Scholar
McKenna, J. and Lyne, A. G. 1988, Timing measurements of the binary millisecond pulsar in the globular cluster M4, Nature, 336, 226–227.Google Scholar
McKinnon, M. M. and Hankins, T. H. 1992, Intensity dependence of the PSR 0329+54 pulse profile, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 191–193.Google Scholar
Melrose, D. B. 1976, Effects of an ambient magnetic field on the properties of Langmuir waves, Solar Phys., 46, 511.Google Scholar
Melrose, D. B. 1978, Amplified linear acceleration emission applied to pulsars, Astrophys. J., 225, 557.CrossRefGoogle Scholar
Melrose, D. B. 1979, Propogation efects on the polarization of pulsar radio emission, Aust. J. Phys., 32, 61.Google Scholar
Melrose, D. B. 1980, Plasma Astrophysics, (New York: Gordon and Breach). 2 vols.Google Scholar
Melrose, D. B. 1981, Maser pulse emission mechanisms, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 133–140.Google Scholar
Melrose, D. B. 1986, Instabilities in Space and Laboratory Plasmas, (Cambridge: Cambridge Univ. Press).CrossRefGoogle Scholar
Melrose, D. B. 1989, The brightness temperaures of solar type III bursts, Solar Phys., 120, 369.Google Scholar
Melrose, D. B. 1992, Coherent radio emission mechanisms for pulsars, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 307–316.Google Scholar
Melrose, D. B. and Dulk, G. A. 1982, Electron-cyclotron masers as the source of certain solar and stellar radio bursts, Astrophys. J., 259, 884.Google Scholar
Melrose, D. B. and Goldman, M. V. 1987, Microstructures in type III events in the solar wind, Solar Phys., 107, 329.Google Scholar
Melrose, D. B. and Parle, A. J. 1983, Quantum electrodynamics in strong magnetic field, Aust. J. Phys., 36, 799.Google Scholar
Melrose, D. B. and Stoneham, R. J. 1977, The natural modes in a pulsar magnetosphere, Proc. Astr. Soc. Aust., 3, 120–122.Google Scholar
Mertz, L. 1974, Mode-locked maser theory of pulsars, Astrophys. Space Sci., 30, 43.Google Scholar
Mestel, L. 1971, Pulsar magnetosphere, Nature Phys. Set., 233, 149.Google Scholar
Mestel, L. 1981, Structure of the pulsar magnetosphere, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 9–23.Google Scholar
Mestel, L., Phillips, P., and Wang, Y. M. 1979, The axisymmetric pulsar magnetosphere - I, Mon. Not. R. astr. Soc., 188, 385–114.CrossRefGoogle Scholar
Mestel, L., Robertson, J. A., Wang, Y. M., and Westfold, K. C. 1985, The axisymmetric pulsar magnetosphere, Mon. Not. R. astr. Soc., 217, 443.Google Scholar
Mestel, L. and Wang, Y. M. 1979, The axisymmetric pulsar magnetosphere - II, Mon. Not. R. astr. Soc., 188, 799–812.Google Scholar
Mészéroe, P. and Riffert, H. 1987, On the radius of neutron stars, Astrophys. J., 323, L30.Google Scholar
Meurs, E. J. A. and van den Heuvel, E. P. J. 1989, The number of evolved early-type close binaries in the galaxy, Astr. Astrophys., 226, 88.Google Scholar
Michel, F. C. 1969, Relativistic stellar wind torques, Astrophys. J., 158, 727.Google Scholar
Michel, F. C. 1972, Accretion of matter by condensed objects, Astrophys. Space Sci., 15, 153–160.Google Scholar
Michel, F. C. 1973, Rotating magnetosphere: A simple relativistic model, Astrophys. J., 180, 207.Google Scholar
Michel, F. C. 1974, Rotating magnetosphere: Acceleration of plasma from the stellar surface, Astrophys. J., 192, 713.Google Scholar
Michel, F. C. 1980, The quiet aligned rotator, Astrophys. Space Sci., 72, 175–181.Google Scholar
Michel, F. C. 1981, Pulsar disk systems, Astrophys. J., 251, 654.Google Scholar
Michel, F. C. 1982, Theory of pulsar magnetospheres, Reviews of Modern Physics, 54, 1–66.Google Scholar
Michel, F. C. 1983, Radio pulsar disk electrodynamics, Astrophys. J., 266, 188–200.Google Scholar
Michel, F. C. 1985, Gamma-ray bursts from remnant neutron star disks, Astrophys. J., 290, 721–727.Google Scholar
Michel, F. C. 1987a, Pulsar activation by the interstellar medium, Astrophys. J., 312, 271.Google Scholar
Michel, F. C. 1987b, A pulsar emission model: Observational tests, Astrophys. J., 322, 822.CrossRefGoogle Scholar
Michel, F. . 1990, submitted to Astrophys. J.Google Scholar
Michel, F. C. 1991, Theory of Neutron Star Magnetospheres, (Chicago: The University of Chicago Press).Google Scholar
Michel, F. C. and Dessler, A. J. 1981, Pulsar disk systems, Astrophys. J., 251, 654–664.Google Scholar
Michel, F. C. and Goldwire, H. C. 1970, Alignment of oblique rotators, Astrophys. J., 5, 21.Google Scholar
Michel, F. C., Scowen, P. A., Dufour, R. J., and Hester, J. J. 1991, Observation of a pulsar wind: CCD photometry of the Crab nebula, Astrophys. J., 368, 463.Google Scholar
Mikhailovskii, A. B., Onishchenko, O. G., and Smolyakov, A. I. 1985, Theory of low-frequency electromagnetic solitons in relativistic electron-positron plasma, Sov. J. Plasma Phys., 11, 215.Google Scholar
Mikhailovskii, A. B., Onishchenko, O. G., Suramlishvili, G. I., and Sharapov, S. E. 1982a, The emergence of electromagnetic waves from pulsar magnetospheres, Sov. Astron. Lett., 8, 369.Google Scholar
Mikhailovskii, A. B., Onishchenko, O. G., Suramlishvili, G. I., and Sharapov, S. E. 1982b, On the problem of the coming out of electromagnetic waves from the magnetosphere of pulsars, Pis'ma Astron. Zh., 8, 685–688.Google Scholar
Mikhailovskii, A. B., Onishchenko, O. G., and Tatarinov, E. G. 1985a, Alfvén solitons in a relativistc electronpositron plasma II. Kinetic theory, Plasma Phys. Contr. Fusion, 27, 539.Google Scholar
Mikhailovskii, A. B., Onishchenko, O. G., and Tatarinov, E. G. 1985b, Alfvén solitons in a relativistc electronpositron plasma I. Hydrodynamic theory, Plasma Phys. Contr. Fusion, 27, 527.Google Scholar
Minkowski, R. 1968, Nonthermal galactic radio sources, in Nebulae and Interstellar Matter, ed. Middlehurst, B. M. and Aller, L. H., (Chicago: University of Chicago Press), 623.Google Scholar
Misner, C. W., Thome, K. S., and Wheeler, J. A. 1973, Gravitation, (San Francisco: W. H. Freeman).Google Scholar
Mofiz, U. A. 1989, Isolated solitons in an ultrarelativistic electron-positron plasma of a pulsar magnetosphere, Phys. Rev., A40, 2203.CrossRefGoogle Scholar
Mofiz, U. A., Bhuiyan, G. M., Ahmed, Z., and Asgar, M. A. 1988, Relativistic excitation of envelope solitons in electron-positron plasmas of the pulsar magnetospheres, Phys. Rev., A38, 5935.Google Scholar
Mofiz, U. A., de Angelis, U., and Forlani, A. 1984, Localized solutions for circularly polarized electromagnetic waves in electron-positron plasmas, Plasma Phys. Contr. Fusion, 26, 1099.Google Scholar
Mofiz, U. A., de Angelis, U., and Forlani, A. 1985, Solitons in weakly nonlinear electron-positron plasmas and pulsar microstructures, Phys. Rev., A31, 951.Google Scholar
Mofiz, U. A. and Podder, J. 1987, Solitons in strongly magnetized electron-positron plasmas and pulsar microstructures, Phys. Rev., A36, 1811.Google Scholar
Morris, D. and Berge, G. L. 1962, Measurements of the polarization and angular extent of the decimeter radiation from Jupiter, Astrophys. J., 136, 276.Google Scholar
Morris, D., Graham, D. A., Seiber, W., Bartel, N., and Thomasson, P. 1981, Observations of the polarization of average pulsar profiles at high frequency, Astr. Astrophys. Suppl. Ser., 46, 421–472.Google Scholar
Müller, D. 1984, Variational calculation of iron and helium atoms and molecular chains in superstrong magnetic fields, Astr. Astrophys., 130, 415.Google Scholar
Murakami, T. et al.. 1988, Evidence for cyclotron absorption from spectral features in gamma-ray bursts seen with Ginga, Nature, 335, 234.Google Scholar
Muslimov, A. G. and Tsygan, A. I. 1985, Neutron star superconductivity and superfluidity and the decay of pulsar magnetic fields, Sov. Astron., L11, 80.Google Scholar
Muslimov, A. G. and Tsygan, A. I. 1986, The electric fields induced by the rotating neutron star in vacuo in General Relativity, Astron. Zh., 63, 958.Google Scholar
Muslimov, A. G. and Tsygan, A. I. 1990a, The effects of General Relativity on the electrodynamics of a pulsar, in Proc. of Adraitic Working Party on Condensed Matter Properties of Neutron Stars (11-29 Sept. 1989 Trieste), (Singapore: World. Sci. Publ.).Google Scholar
Muslimov, A. G. and Tsygan, A. I. 1990b, The influence of general relativistic effects on the electrodynamics of neutron stars, Astron. Zh., 67, 263.Google Scholar
Nagase, F. 1989, Accretion-powered x-ray pulsars, Publ. Astron. Soc. Japan, 41, 1.Google Scholar
Narayan, R. 1987, The birthrate and initial spin period of single radio pulsars, Astrophys. J., 319, 162–179.Google Scholar
Narayan, R. and Ostriker, J. P. 1990, Pulsar populations and their evolution, Astrophys. J., 352, 222–246.Google Scholar
Narayan, R. and Vivekanand, M. 1981, A lower limit for the birthrate of pulsars, Nature, 290, 571–572.Google Scholar
Narayan, R. and Vivekanand, M. 1982, Geometry of pulsar beams: Relative orientation of rotation axis, magnetic axis and line of sight, Astr. Astrophys., 113, L3–L6.Google Scholar
Narayan, R. and Vivekanand, M. 1983, Evidence for evolving elongated pulsar beams, Astr. Astrophys., 122, 45–53.Google Scholar
Neider, J. A. and Mead, R. 1965, A simplex method for function minimization, Computer Journal, 7, 308–313.Google Scholar
Nelson, R. and Wasserman, I. 1989, Resonant mode-mode coupling in torsional oscillations of neutron stars, Bull. American Astron. Soc., 20, 1349.Google Scholar
Neuhauser, D., Koonin, S. E., and Langanke, K. 1987, Hartree-Fock calculations of atoms and molecular chains in strong magnetic fields, Phys. Rev., A36, 4163.Google Scholar
Nomoto, K., Shigeyama, T., Kumagai, S., and Hashimoto, M. 1988, New developments in theoretical modelling of SN 1987A, Proc. Astr. Soc. Aust., 7, 490–504.Google Scholar
Nomoto, K. and Tsuruta, S. 1987, Cooling of neutron stars: Effects of the finite time scale of thermal conduction, Astrophys. J., 312, 711.Google Scholar
Novikov, A. Y., Popov, M. V., Smirnova, T. V., and Soglasnov, V. A. 1983, Sov. Astron., 60, 280.Google Scholar
Nowakowski, L. A. 1991, PSR 0540+23 revisited: Three components, drifting subpulses and mode switching, Astrophys. J., 377, 581–587.Google Scholar
Nowakowski, L. A. and Hankins, T. H. 1985, preprint.Google Scholar
Ochelkov, Y. P. and Usov, V. V. 1980, Curvature radiation of relativistic particles in the magnetosphere of pulsars I. Theory, Astrophys. Space Sci., 69, 439–460.Google Scholar
Ü;gelman, H., Fichtel, C. E., Kniffen, D. A., and Thompson, D. J. 1976, A search of the SAS-2 data for the pulsed gamma-ray emission from radio pulsars, Astrophys. J., 209, 584.Google Scholar
Ü;gelman, H. and Zimmerman, H. U. 1989, Soft X-ray observations of the Vela pulsar PSR0833-45, Astr. Astrophys., 214, 179–185.Google Scholar
Okamoto, I. 1974, Force free pulsar magnetosphere - I. The steady axisymmetric theory from the charge separated plasma, Mon. Not. R. astr. Soc, 167, 457.Google Scholar
Onischenko, O. G. 1981, On the theory of orthogonal modes in pulsar radio emission, Sov. Astron. Lett., 7, 731.Google Scholar
Ostriker, J. P. and Gunn, J. E. 1969, On the nature of pulsars: I. Theory., Astrophys. J., 157, 1395.Google Scholar
Ostriker, J. P., Rees, M. J., and Silk, J. I. 1970, Some observable consequences of accretion by defunct pulsars, Astrophys. Lett., 6, 179–184.Google Scholar
Ott, E., Antonsen, T. M., and Lovelace, R. V. 1977, Theory of foil-less diode generation of intense relativistic electron beams, Phys. Fluids, 20, 1180.Google Scholar
Pacini, F. 1967, Energy emission from a neutron star, Nature, 216, 567–568.Google Scholar
Packard, N. H., Crutchfield, J. P., Farmer, J. D., and Shaw, R. S. 1980, Geometry from a time series, Phys. Rev. Lett., 45, 712.Google Scholar
Paczyński, B. 1981, Evolution of cataclysimic binaries, Acta. Astron., 31, 1–12.Google Scholar
Page, C. G. 1973, The drifting subpulse phenomenon in PSR 0809+74, Mon. Not. R. astr. Soc., 163, 29–40.CrossRefGoogle Scholar
Pandharipande, V. R. 1971a, Dense neutron matter with realistic interactions, Nucl. Phys., A174, 641–656.Google Scholar
Pandharipande, V. R. 1971b, Hyperionic matter, Nucl. Phys., A178, 123–144.Google Scholar
Pataraya, A. and Melikidze, G. 1980, Modulational instability of nonlinear waves in the relativistic plasma with account of the nonlinear Landau damping, Astrophys. Space Sci., 68, 61.Google Scholar
Pekerie, C. L., Alterman, Z., and Jarosch, H. 1961, Phys. Rev., 122, 1692.Google Scholar
Pellat, R. 1979, Theoretical aspects of coherent radioemission in nature: The pulsar example, Space Sci. Rev., 24, 601.Google Scholar
Pelletier, G., Sol, H., and Asséo, E. 1988, Magnetized Langmuir wave packets excited by a strong beam-plasma interaction, Phys. Rev., 38, 2552.Google Scholar
Pelling, R. M., Paciesas, W. S., Peterson, L. E., Makashima, K., Oda, M., Ogawara, Y., and Miyamoto, S. 1987, A scanning modulation collimator observation of the high energy x-ray source in the Crab nebula, Astrophys. J., 319, 416.Google Scholar
Petschek, H. E. 1964, Physics of solar flares, in AAS-NASA Symp. Physics of Solar Flares, (Washington D. C.: NASA Publications SP-50), 425.Google Scholar
Petschek, H. E. and Thorne, R. M. 1967, The existence of intermediate waves in neutral sheets, Astrophys. J., 147, 1157.Google Scholar
Phillips, J. A. 1990, The magnetic geometry and radio beam of PSR 1929+10, Astrophys. J., 361, L57.Google Scholar
Phillips, J. A. and Wolszczan, A. 1989, Interpulse emission from pulsars at 25 MHz, Astrophys. Lett., 344, L69.Google Scholar
Phillips, J. A. and Wolszczan, A. 1990, Pulsar astronomy at meter and decameter wavelengths: Results from Arecibo, in Low Frequency Radio Astronomy from Space, ed. Weiler, K. and Kassim, N., (New York: Springer-Verlag Lecture Notes in Physics Series), 175.Google Scholar
Piddington, J. H. 1957, The Crab nebula and the origin of interstellar magnetic fields, Aust. J. Phys., 10, 530.Google Scholar
Pines, D. 1980, Pulsars and compact X-ray sources—cosmic laboratories for the study of neutron stars and hadrom matter, Uap. Fiz. Nauk., 131, 479–494.Google Scholar
Popov, M. V. and Smirnova, T. V. 1982, The drift behavior of PSR 0809+74, Sov. Astron., 26, 439–442.Google Scholar
Popov, M. V., Smirnova, T. V., and Soglasnov, V. A. 1987, Study of the microstructure of pulsars PSR 0809+74, 0950+08 and 1133+16 in a frequency range 67 - 102MHz, Sov. Astron., 31(5), 529.Google Scholar
Popov, M. V., Smirnova, T. V., Soglasnov, V. A., and Novikov, A. Y. 1985, Sov. Astron., 62, 561.Google Scholar
Press, W. H., Flannery, B. P., Teukolsky, S. A., and Vetterling, W. T. 1986, Numerical Recipes: The Art of Scientific Computing, (New York: Cambridge University Press).Google Scholar
Prószyński, M. and Przybycień, D. 1984, Pulsar statistics: a study of pulsar luminosities, in Millisecond pulsars, ed. Reynolds, S. P. and Stinebring, D. R., (Green Bank: NRAO), 151–157.Google Scholar
Prószyński, M. A. 1979, Geometry fo pulsar emission and pulse width statistics, Astr. Astrophys., 79, 8.Google Scholar
Qiao, G. J. 1988a, Inverse-Compton Scattering plays an important role in pulsar emission, in High Energy Astrophysica, ed. Borner, G., (New York: Springer-Verlag), 88.Google Scholar
Qiao, G. J. 1988b, A mechanism for core emission of pulsars, Vistas Astro., 31, 393.Google Scholar
Qiao, G. J. 1992, The radiation beams and the pulse profiles of pulsars in an Inverse Compton Scattering (ICS) model, in The Magnetospheric Structure and Emission Mechaniams of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 239–242.Google Scholar
Qiao, G. J., Li, C. G., and Li, M. 1992, The locations of the core and conal emission regions in an Inverse-Compton Scattering model, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 243–245.Google Scholar
Qiao, G. J., Wu, X. J., Bao, W., and Xia, X. Y. 1986, Inverse Compton Scattering in strong magnetic fields and optical emission of the Crab pulsar, Scientia Sinica, 7, 732.Google Scholar
Radhakrishnan, V. 1969, Fifteen months of pulsar astronomy, Proc. Astr. Soc. Aust., 1, 254.Google Scholar
Radhakrishnan, V. 1982, On the nature of pulsars, Contemp. Phys., 23, 207–231.Google Scholar
Radhakrishnan, V. and Cooke, D. J. 1969, Magnetic poles and the polarization structure of pulsar radiation, Astrophys. Lett., 3, 225.Google Scholar
Radhakrishnan, V. and Rankin, J. M. 1990, Toward an empirical theory of pulsar emission: V. On the circular polarization in pulsar radiation, Astrophys. J., 352, 258–266.Google Scholar
Ramaty, R., Bonazzola, S., Cline, T. L., Kazanas, D., and Mészáros, P. 1980, Origin of the 5 March 1979 gamma-ray transient: a vibrating neutron star, Nature, 287, 122–124.CrossRefGoogle Scholar
Rankin, J. M. 1983a, Toward an empirical theory of pulsar emission: I. Morphological taxonomy, Astrophys. J., 274, 333–358.Google Scholar
Rankin, J. M. 1983b, Toward an empirical theory of pulsar emission: II. On the spectral behavior of component width, Astrophys. J., 274, 359–368.Google Scholar
Rankin, J. M. 1986, Toward an empirical theory of pulsar emission: III. Mode changing, drifting subpuises and pulse nulling, Astrophys. J., 301, 901–922.Google Scholar
Rankin, J. M. 1988, On the polarization modal construction of triplicity in the profile of pulsar PSR 1604-00, Astrophys. J., 325, 314–319.Google Scholar
Rankin, J. M. 1990, Toward an empirical theory of pulsar emission: IV. Geometry of the core emission region, Astrophys. J., 352, 247.Google Scholar
Rankin, J. M. 1992, On the primary importance of pulsars with five-component profiles, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 196–201.Google Scholar
Rankin, J. M., Campbell, D. B., and Backer, D. C. 1974, Individual pulse polarization properties of three pulsars, Astrophys. J., 188, 609–613.Google Scholar
Rankin, J. M., Cornelia, J. M., Craft, H. D. Jr., Richards, D. W., Campbell, D. W., and Counselman, C. C. 1970, Radio pulse shapes, flux densities, and dispersion of pulsar NP 0532, Astrophys. J., 162, 707–725.Google Scholar
Rankin, J. M. and Gil, J. A. 1989, Phenomenology and the problem of pulsar emission, Comments in Astrophysics, 14, 1–10.Google Scholar
Rankin, J. M., Stinebring, D. R., and Weisberg, J. M. 1989, Arecibo 21-cm polarimetry of 64 pulsars: A guide to classification, Astrophys. J., 346, 869–897.Google Scholar
Rankin, J. M., Wolszczan, A., and Stinebring, D. R. 1988, Mode changing and quasi-periodic modulation in pulsar 1737+13, a bright, five-component pulsar, Astrophys. J., 324, 1048–1055.Google Scholar
Rappaport, S., Putney, A., and Verbunt, F. 1989, Evolution of wide binary millisecond pulsars in globular clusters, Astrophys. J., 345, 210–221.Google Scholar
Rawley, L. A., Taylor, J. H., and Davis, M. M. 1988, Fundamental astrometry and millisecond pulsars, Astrophys. J., 326, 947–953.Google Scholar
Rawley, L. A., Taylor, J. H., Davis, M. M., and Allan, D. W. 1987, Millisecond pulsar PSR 1937+21: A highly stable clock, Science, 238, 761.Google Scholar
Rees, M. J. and Gunn, J. E. 1974, The origin of the magnetic field and relativistic particles in the Crab nebula, Mon. Not. R. oatr. Soc, 167, 1.Google Scholar
Reynolds, R. J. 1989, The column density and scale height of free electrons in the galactic disk, Astrophys. J., 339, L29.Google Scholar
Rickett, B. J. 1975, Amplitude-modulated noise: An empirical model for the radio radiation received from pulsars, Astrophys. J., 197, 185–191.Google Scholar
Rickett, B. J. 1977, Interstellar scattering and scintillation of radio waves, Ann. Rev. Astr. Ap., 15, 479–504.Google Scholar
Rickett, B. J. and Cordes, J. M. 1981, The location, spectrum and beamwidth of pulsar radiation from polar cap models, in Pulsars, 13 Years of Research on Neutron Stars, JA U Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 107–109.Google Scholar
Rickett, B. J., Hankins, T. H., and Cordes, J. M. 1975, The radio spectrum of micropulses from pulsar PSR 0950+08, Astrophys. J., 201, 425–430.Google Scholar
Ritchings, R. T. 1976, Pulsar single pulse intensity measurements and pulse nulling, Mon. Not. R. astr. Soc., 176, 249–263.Google Scholar
Rizzato, F. B. 1988, Weakly nonlinear electromagnetic waves and low-frequency magnetic field in electron-positronion plasmas, J. Plasma Phys., 40, 289.Google Scholar
Rizzato, F. B., Schneider, R. S., and Dillenburg, D. 1988, Electromagnetic solitons in a strongly magnetized electron-positron-ion plasma, Phys. Lett., A133, 59.Google Scholar
Romani, R. W. 1990a, Binary periods of cluster pulsars, Astrophys. J., 357, 493–501.Google Scholar
Romani, R. W. 1990b, A unified model of neutron-star magnetic fields, Nature, 347, 741.Google Scholar
Romani, R. W. and Hernquist, L. E. 1992, Evolution of thermally generated neutron-star magnetic fields, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 46–48.Google Scholar
Rowe, E. T. 1990, A linear acceleration emission mechanism, Proc. Astr. Soc. Aust., 8, 357–359.Google Scholar
Rowe, E. T. 1992, Linear acceleration emission: A detailed analysis, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 123–129.Google Scholar
Ruderman, M. 1970, Long period oscillations in rotating neutron stars, Nature, 225, 619–620.Google Scholar
Ruderman, M. 1971, Matter in superstrong magnetic fields: The surface of a neutron star, Phys. Rev. Lett., 27, 1306–1308.Google Scholar
Ruderman, M. A. 1981, Evolution and radiation in pulsar polar cap models, in Pulsars, 13 Years of Research on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 87–98.Google Scholar
Ruderman, M. A. 1985, Cosmogonical Processes, (Utrecht: VNU Sciena Press).Google Scholar
Ruderman, M. A. 1987, Energetic radiation from magnetized neutron stars, in High energy phenomena around collapsed stars. Proceedings of a NATO Advanced Study Institute, ed. Pacini, F., (Dordrecht: D. Reidel).Google Scholar
Ruderman, M. A. and Sutherland, P. G. 1973, Possible origin of magnetic field in neutron stars and magnetic white dwarfs, Nature Phys. Sci., 246, 93.Google Scholar
Ruderman, M. A. and Sutherland, P. G. 1975, Theory of pulsars: Polar gaps, sparks, and coherent microwave radiation, Astrophys. J., 196, 51.Google Scholar
Ruelle, D. 1981, In nonlinear phenomena in chemical dynamics, (Berlin: Springer-Verlag).Google Scholar
Rylov, Y. A. 1976, Electron and proton regions in the magnetosphere of a charged rotating neutron star with a strong magnetic field, Sov. Astron., 20, 23.Google Scholar
Rylov, Y. A. 1977, On the electron cap shape of a rotating neutron star, Astrophys. Space Sci., 51, 59.Google Scholar
Rylov, Y. A. 1978, On a klystron mechanism of generation of vibrations in pulsar magnetospheres, Astrophys. Space Sci., 53, 377–402.Google Scholar
Rylov, Y. A. 1979, Acceleration of electrons in an internal zone of the pulsar polar cap, Astrophys. Space Sci., 66, 401–428.Google Scholar
Rylov, Y. A. 1981, Electron-positron pair production in the pulsar magnetosphere, Astrophys. Space Sci., 75, 423.Google Scholar
Rylov, Y. A. 1982, The production mechanism of electron-positron bunches in a pulsar magnetosphere and their thermal radio emission, Astrophys. Space Sci., 88, 173–184.Google Scholar
Rylov, Y. A. 1984, Influence of electron-positron pair production on a pulsar magnetosphere structure, Astrophys. Space Sci., 107, 381.Google Scholar
Rylov, Y. A. 1985, The structure of polar caps and the equatorial belt of pulsars, Astrophys. Space Sci., 117, 5.Google Scholar
Rylov, Y. A. 1987, Computer simulation of the particle acceleration in pulsar magnetospheres, Astrophys. Space Sci., 132, 353.Google Scholar
Rylov, Y. A. 1988, Self-consistent model of the global structure of axially-symmetric pulsar magnetosphere in masslees approximation, Astrophys. Space Sci., 143, 269.Google Scholar
Rylov, Y. A. 1989, The algebraical structure of the electro-magnetic tensor and description of charged particles moving in the strong electromagnetic field, J. Math. Phys., 30, 521.Google Scholar
Rylov, Y. A. 1990, Conditions on two-phase boundary in the massless electron-positron gas, Izvestiya Akademii Nauk SSSR. Mechanika shidkocti i gaza, 1, 165. (in Russian).Google Scholar
Sagdeev, R. Z. and Shafranov, V. D. 1960, On the instability of a plasma with an anisotropic distribution of velocities in a magnetic field, Soviet Phys. JETP, 39, 181.Google Scholar
Sakai, J. I. and Kawata, T. 1980a, Nonlinear Alfvén waves in an ultrarelativistic electron-positron plasma, J. Phys. Soc. Japan, 49, 753.Google Scholar
Sakai, J. I. and Kawata, T. 1980b, Waves in an ultrarelativistic electron-positron plasma, J. Phys. Soc. Japan, 49, 747.Google Scholar
Sang, Y. and Chanmugam, G. 1987, Ohmic decay of crustal neutron star magnetic fields, Astrophys. J., 323, L61–L64.Google Scholar
Sauls, J. A. 1989, Superfluidity in neutron stars, in Timing Neutron Stars, (NATO ASI series), ed. Ögelman, H. and Heuvel, E. P. J. van den, (Dordrecht: Kluwer), 457–490.Google Scholar
Sauls, J. A. 1990, in Condensed Matter Properties of Neutron Stars, ed. Srinivasan, G., (Singapore: World Scientific).Google Scholar
Savonije, G. J. 1983, Evolution and mass transfer in X-ray binaries, in Accretion-Driven Stellar X-Ray Sources, ed. Lewin, W. H. G. and Heuvel, E. P. J. van den, (Cambridge: Cambridge University Press), 343.Google Scholar
Scargle, J. D. 1969, Activity in the Crab nebula, Astrophys. J., 156, 401.Google Scholar
Scharlemann, E. T. 1974, Aligned rotating magnetospheres: II. Inclusion of inertial forces, Astrophys. J., 193, 217.Google Scholar
Scharlemann, E. T., Arons, J., and Fawley, W. M. 1978, Potential drops above pulsar polar caps: Ultrarelativistic particle acceleration along the curved magnetic field, Astrophys. J., 222, 297.Google Scholar
Scharlemann, E. T. and Wagoner, R. V. 1973, Aligned rotating magnetospheres: I. General analysis, Astrophys. J., 182, 951.Google Scholar
Schiff, L. I. 1946, Production of particle energies beyond 200 MeV, Rev. Sci. Instr., 17, 6–14.Google Scholar
Schmidt, G. D., Angel, J. R. P., and Beaver, E. A. 1979, The small-scale polarization of the Crab nebula, Astrophys. J., 227, 106–113.Google Scholar
Schmitz, F. H. and Yu, Y. H. 1986, Helicopter impulsive noise: Theoretical and experimental status, J. Sound Vib., 109, 361.Google Scholar
Schott, G. A. 1912, Electromagnetic Radiation, (Cambridge: Cambridge University Press).Google Scholar
Schwinger, J., Tsai, W. Y., and Erber, T. 1976, Classical and quantum theory of synergie Synchrotron-Cherenkov radiation, Ann. Phys. (N. Y.), 96, 303.Google Scholar
Sedrakian, D. M. and Movsissian, A. G. 1986, The magnetic moments of neutron stare with various equations of state, Astrofizica, 24, 279.Google Scholar
Segelstein, D. J., Rawley, L. A., Stinebring, D. R., Fruchter, A. S., and Taylor, J. H. 1986, New millisecond pulsar in a binary system, Nature, 322, 714.Google Scholar
Seiber, W., Reinecke, R., and Wielebinski, R. 1975, Observation of pulsars at high frequencies, Astr. Astrophys.. 38, 169–182.Google Scholar
Seward, F. D. and F. R. Harnden, J. 1982, A new, fast x-ray pulsar in the supernova remnant MSH 15–52, Astrophys. J., 256, L45–L47.Google Scholar
Seward, F. D. and Wang, Z. R. 1988, Pulsars, x-ray synchrotron nebulae and guest stars, Astrophys. J., 332, 199–205.Google Scholar
Shabad, A. E. 1975, Photon dispersion in a strong magnetic field, Ann. Phys. N. Y., 90, 166.Google Scholar
Shabad, A. E. 1988, Polarization of vacuum and quantum relativistic gas, in Proc. of the Lebedev Institute, ed. Ginzburg, V. L., volume 192, (Moscow: Nauka), 5.Google Scholar
Shabanova, T. V. 1990, Results of pulsar timing observations at 102.5 MHz, Sov. Astron., 34(3), 269–274.Google Scholar
Shafranov, V. D. 1963, Voprosi teorii plazmi, Gosatomizdat, 3, 3. in Russian.Google Scholar
Shankar, N. U. and Shankar, T. S. R. 1990, A digital correlation receiver for the Gee Tee radiotélescope, J. Astrophys. Astr., 11, 297–310.Google Scholar
Shapiro, S. L., Teukolsky, S. A., and Washerman, I. 1983, Implications of the millisecond pulsar for neutron star models, Astrophys. J., 272, 702–707.Google Scholar
Shaposhnikov, V. E. 1981, Curvature radiation on longitudinal waves in the magnetosphere of a neutron star, Astrophysics, 17, 407.Google Scholar
Shibata, S. 1990, A DC circuit model of a pulsar magnetosphere, Astrophys. J., in press.Google Scholar
Shibazaki, N. and Lamb, F. K. 1989, Neutron star evolution with internal heating, Astrophys. J., 346, 808–822.Google Scholar
Shibazaki, N., Murakami, T., Shaham, J., and Nomoto, K. 1989, Does mass accretion lead to field decay in neutron stars, Nature, 342, 656.Google Scholar
Shitov, Y. P. 1971, Characteristic of pulsars radio emission at meter wavelengths. PhD thesis, Lebedev Physical Institute, Moscow.Google Scholar
Shitov, Y. P. 1983, The dependence of the spectrum on the period and the twist effect of the pulsar magnetic field, Sov. Aatron., 27, 314–321.Google Scholar
Shitov, Y. P. 1985, Superdispersion pulse delay of the pulsar PSR 0809+74 at meter wavelengths, Sov. Astron. Lett., 11, 94.Google Scholar
Shitov, Y. P., Malofeev, V. M., and Izvekova, V. A. 1988, Superdispersion delay of low-frequency pulsar pulses, Sov. Astron. Lett.. 14, 181.Google Scholar
Shklovskii, I. S. 1970, Pulsar NP 0532; An injection of relativistic particles in Crab nebula, Astrophys. J., 159, L77–L80.Google Scholar
Shukla, P. K. 1985, Self-modulation of pulsar radiation in strongly magnetized electron-positron plasmas, Astrophys. Space Sci., 114, 381.Google Scholar
Shukla, P. K., Rao, N. N., Yu, M. Y., and Tsintsadze, N. L. 1986, Relativistic nonlinear effects in plasmas, Phys. Reports, 138, 1.Google Scholar
Shull, J. M., Fesen, R. A., and Saken, J. M. 1989, Pulsar reenergization of old supernova remnant shells, Astrophys. J., 346, 860–868.Google Scholar
Sieber, W. and Oster, L. 1975, Drifting subpulse behavior of PSR's 0943+10 and 2303+30, Astr. Astrophys., 38, 325–327.Google Scholar
Sieber, W. and Wielebinski, R. 1987, Pulsar characteristics at 24 GHz, Astr. Astrophys., 177, 342.Google Scholar
Silin, V. P. 1960, On the electromagnetic properties of a relativistic plasma, Soviet Phys. JETP, 11(5), 1136.Google Scholar
Slee, O. B., Bobra, A. D., and Alurkar, S. K. 1987, Spectral behavior of pulse width in pulsars, Aust. J. Phys., 40, 557–586.Google Scholar
Smirnova, T. V. 1983, Instantaneous drift-rate dependence of pulsar subpulse energies, Sov. Astron., 27, 80–83.Google Scholar
Smirnova, T. V. and Shabanova, T. V. 1986. Preprint No. 31, Lebedev Physical Institute, USSR, Academy of Sciences, Moscow (in Russian).Google Scholar
Smirnova, T. V. and Shabanova, T. V. 1989, Interpulse radioemission of pulsars, in Proc. FIAN, volume 199, 68.Google Scholar
Smirnova, T. V. and Shishov, V. I. 1989, The spatial structure of the emission sources of pulsar PSR 1133+16, Astron. Zh., 15, 443.Google Scholar
Smirnova, T. V., Soglasnov, V. A., Popov, M. V., and Novikov, A. Y. 1986, Dual-frequency correlation of pulsar micropulses, Sov. Astron., 30, 51–56.Google Scholar
Smith, A. and Pounds, K. A. 1977, X-ray flare in 3U 0833-45, the Vela pulsar, Nature, 265, 121.Google Scholar
Smith, F. G. 1974, Counter-rotation of polarization vectors in pulsars, Mon. Not. R. astr. Soc., 167, 43P-46P.Google Scholar
Smith, F. G. 1977, Pulsars, (Cambridge: Cambridge University Press).Google Scholar
Smith, F. G. 1986, The geometry of the emission from the Vela and Crab pulsars, Mon. Not. R. astr. Soc., 219, 729–736.Google Scholar
Soglasnov, V. A., Popov, M. V., and Kuz'min, A. D. 1983 A statistical analysis of the fine-scale time structure of PSR 1133+16, Sov. Astron., 27(2), 169–173.Google Scholar
Soglasnov, V. A., Smirnova, T. V., Popov, M. V., and Kuz'min, A. D. 1981, Statistical analysis of the temporal fine structure of the pulsar PSR 0809+74, Sov, Astron., 25, 442–445.Google Scholar
Sonin, E. B. 1987, Vortex oscillations and hydrodynamics of rotating superfluids, Reviews of Modern Physics, 59, 87–155.Google Scholar
Spitzer, L. 1987, Dynamical Evolution of Globular Clusters, (Princeton: Princeton University Press).Google Scholar
Srinivasan, G. 1989, Pulsars: their origin and evolution, Astron. Ap. Rev., 1, 209.Google Scholar
Srinivasan, G., Bhattacharya, D., Muslimov, A. G., and Tsygan, A. I. 1990, A novel mechanism for the decay of neutron star magnetic fields, Curr. Sci., 59, 31.Google Scholar
Staelin, D. H. and Reifenstein, E. C. III 1968, Pulsating radio sources near the Crab Nebula, Science, 162 1481–1483.Google Scholar
Staelin, D. H. and Sutton, J. M. 1970, Observed shapes of Crab Nebula radio pulses, Nature, 226, 69–70.Google Scholar
Stenflo, L., Shukla, P. K., and Yu, M. Y. 1985, Nonlinear propogation of electromagnetic waves in magnetized electron-positron plasmas, Astrophys. Space Sci., 117, 303.Google Scholar
Stinebring, D. R. 1982, Pulsar polarization: Dual-frequency observations and the production of orthogonally polarized radiation. PhD thesis, Cornell University.Google Scholar
Stinebring, D. R. and Condon, J. J. 1990, Pulsar flux stability and refractive interstellar scintillation, Astrophys. J., 352, 207.Google Scholar
Stinebring, D. R., Cordes, J. M., Rankin, J. M., Weisberg, J. M., and Boriakoff, V. 1984a, Pulsar polarization fluctuations: I. 1408 MHz statistical summaries, Astrophys. J. Supp. Series, 55, 247–277.Google Scholar
Stinebring, D. R., Cordes, J. M., Weisberg, J. M., Rankin, J. M., and Boriakoff, V. 1984b, Pulsar polarization fluctuations: II. 800 MHz statistical summaries, Astrophys. J. Supp. Series, 55, 279–288.Google Scholar
Stinebring, D. R., Ryba, M. F., Taylor, J. H., and Romani, R. W. 1990, Cosmic gravitational-wave background: Limits from millisecond pulsar timing, Phys. Rev. Lett., 65, 285–288.Google Scholar
Stollman, G. M. 1987, The radio luminosity of pulsars, Astr. Astrophys., 171, 152–156.Google Scholar
Stoneham, R. J. 1981, Pulsar optical emission as amplified synchrotron emission, in Pulsars, 13 Years of Reaearch on Neutron Stars, IAU Symposium No. 95, ed. Sieber, W. and Wielebinski, R., (Dordrecht: D. Reidel), 235–238.Google Scholar
Sturrock, P. A. 1971, A model of pulsars, Astrophys. J., 164, 529.Google Scholar
Sturrock, P. A., Harding, A. K., and Daugherty, J. K. 1989, Cascade model of gamma-ray bursts, Astrophys. J., 346, 950–959.Google Scholar
Sturrock, P. A., Petrosian, V., and Turk, J. S. 1975, Optical radiation from the Crab pulsar, Astrophys. J., 196, 73.Google Scholar
Suleymanova, S. A. 1989, Linear polarization of averaged pulses at frequencies of 102.5, 60 and 40 MHz, Proceedings of the Lebedev Institute, 199, 42.Google Scholar
Suleymanova, S. A. and Izvekova, V. A. 1984, The detection of two modes in the radiation of the pulsar PSR 0943+10 at the meter wave lengths, Sov. Astron., 28, 32–35.Google Scholar
Sutton, J. M., Staelin, D. H., Price, R. M., and Weiner, R. 1970, Three pulsars with marching subpulses, Astrophys. J., 159, L89.Google Scholar
Suvorov, E. V. and Chugunov, Y. V. 1975, Electromagnetic waves in a relativistic plasma with a strong magnetic field, Astrophysics, 11, 203.Google Scholar
Suvorov, E. V. and Chugunov, Y. V. 1980, Longitudinal waves in a relativistic plasma, Sov. J. Plasma Phys., 6, 69.Google Scholar
Svetozarova, G. I. and Tsytovitch, V. N. 1962, On the space dispersion of relativistic plasma in magnetic field, Izv. Vuzov. Radiofizika, 5, 658.Google Scholar
Taam, R. E. and van den Heuvel, E. P. J. 1986, Magnetic field decay and the origin of neutron star binaries, Astrophys. J., 305, 235–245.Google Scholar
Tademaru, E. 1973, On the energy spectrum of relativistic electrons in the Crab nebula, Astrophys. J., 183, 625.Google Scholar
Taylor, J. H. and Dewey, R. J. 1988, Improved parameters for four binary pulsars, Astrophys. J., 332, 770–776.Google Scholar
Taylor, J. H. and Huguenin, G. R. 1971, Observations of rapid fluctuations of intensity and phase in pulsar emissions, Astrophys. J., 167, 273.Google Scholar
Taylor, J. H., Huguenin, G. R., Hirsch, R. M., and Manchester, R. N. 1971, Polarization of the drifting subpulses of pulsar 0809+74, Astrophys. Lett., 9, 205–208.Google Scholar
Taylor, J. H. and Manchester, R. N. 1975, Observed properties of 147 pulsars, Astron. J., 80, 794.Google Scholar
Taylor, J. H. and Manchester, R. N. 1977, Galactic distribution and evolution of pulsars, Astrophys. J., 215, 885–896.Google Scholar
Taylor, J. H., Manchester, R. N., and Huguenin, G. R. 1975, Observations of pulsar radio emission: I. Totalintensity measurements of individual pulses, Astrophys. J., 195, 513.Google Scholar
Taylor, J. H. and Stinebring, D. R. 1986, Recent progress in the understanding of pulsars, Ann. Rev. Astr. Ap., 24, 285–327.Google Scholar
Taylor, J. H. and Weisberg, J. M. 1982, A new test of general relativity: Gravitational radiation and the binary pulsar PSR 1913+16, Astrophys. J., 253, 908–920.Google Scholar
Taylor, J. H. and Weisberg, J. M. 1989, Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16, Astrophys. J., 345, 434–450.Google Scholar
Thielheim, K. O. 1986, Cosmic ray particle acceleration in pulsar magnetospheres, in The Origin and Evolution of Neutron Stars, Proc. IAU Symp. No. 125, ed. Helfand, D. J. and Huang, J. H., (Dordrecht: D. Reidel), 555.Google Scholar
Thielheim, K. O. 1989, Fundamentals of Cosmic Physics, 13, 357–399.Google Scholar
Thielheim, K. O. and Tolan, M. 1990, to be published.Google Scholar
Thompson, D. J. and Kniffen, D. A. 1989, Gamma-ray pulsars: Prospects and limitations, in Proceedings of the Gamma Ray Obaervatory Science Workshop, ed. Johnson, W. N., (Washington: Naval Research Laboratory), 4–150.Google Scholar
Thorne, K. S. 1978, General relativistic astrophysics, in Theoretical Principlea in Astrophysica and Relativity, ed. Lebovitz, N. R., Reid, W. H., and Vandervoort, P. O., (Chicago: Univ. of Chicago Press), 149–216.Google Scholar
Thorsett, S. E. 1991, Frequency dependence of pulsar integrated profiles, Astrophys. J., 377, 263–267.Google Scholar
Thorsett, S. E. and Stinebring, D. R. 1990, Polarimetry of millisecond pulsars, Astrophys. J., 361, 644.Google Scholar
Trümper, J., Pietsch, W., Reppin, C., Voges, W., Staubert, R., and Kendziorra, E. 1978, Evidence for strong cyclotron line emission in the hard x-ray spectrum of Hercules X-1, Astrophys. J., 219, L105.Google Scholar
Tsuruta, S. 1979, Cooling and heating of neutron stars. Current status, in Proc. Intern. School of Physics, Enrico Fermi Courae LXV, Varenna, 635.Google Scholar
Tsuruta, S. 1985, Neutron stars: Current cooling theories and observational reaulta, (Munich: Max Planck Institut für Astrophysik). Preprint M PA.Google Scholar
Tsuruta, S. 1987, Neutron star cooling, in Proc. of 13th Texas Symp. on Rel. Astrophys., ed. Ulmer, M., (Singapore: World Scientific), 499–503.Google Scholar
Tsytovich, V. N. and Kaplan, S. A. 1972, Relativistic plasma and pulsar emission mechanisms, Nature Phys. Sci., 241, 122.Google Scholar
Turner, P. J. 1980, Low Dispersion Pulsars. PhD thesis, University of Tasmania.Google Scholar
Twiss, R. Q. 1958, Radiation transfer and the possibility of negative absorption in radio astronomy, Aust. J. Phys., 11, 564.Google Scholar
Ulyanov, O. M. 1989, in Abstracts of XXII YERAC, (Kharkov: ), 23.Google Scholar
Ulyanov, O. M. 1990, An aberration, retardation and twist effect by the pulsars radio emission observation, Kinematics and physics of the celestial bodies, in press.Google Scholar
Unno, W., Osaki, Y., Ando, H., and Shibahashi, H. 1979, Nonradial Oscillations of Stars, (Tokyo: University of Tokyo Press).Google Scholar
Usov, V. V. 1987a, On two-stream instability in pulsar magnetospheres, Astrophys. J., 320, 333.Google Scholar
Usov, V. V. 1987b, Two-stream instability and generation of Langmuir oscillations in pulsar magnetospheres, Sov. Astr. Circ. No. 1431. Google Scholar
Uetimenko, B. Y. 1983, Investigations of radioemission of pulsars in the decametric wave-band. PhD thesis, Kharkov, (in Russian).Google Scholar
van den Heuvel, E. P. J. 1984, Models for the formation of binary and millisecond radio pulsars, J. Astrophys. Astr., 5, 209–233.Google Scholar
van den Heuvel, E. P. J., van Paradijs, J. A., and Taam, R. E. 1986, Evidence for an asymptotic lower limit to the surface dipole magnetic field strengths of neutron stars, Nature, 322, 153–155.Google Scholar
van Horn, H. M. 1980, Micropulses, drifting subpulses and nonradial oscillations of neutron stars, Astrophys. J., 236, 899–903.Google Scholar
Van Paradijs, J. 1989, Gamma-ray bursts and decay of neutron star magnetic fields, Mon. Not. R. astr. Soc., 238, 45P.Google Scholar
Van Riper, K. A. and Lamb, D. Q. 1981, Neutron star evolution and results from the Einstein X-ray observatory, Astrophys. J., 244, L13.Google Scholar
Vasyliunas, V. M. 1975, theoretical models of magnetic field line merging, I, Reviews of Geophysics and Space Physics, 13, 303–336.Google Scholar
Vdovin, A. S., Ilyasov, Y. P., Oreshko, V. V., and Fedorov, Y. A. 1989, Time service for the pulsar time scale, Time and frequency measurements, VNIIFTRI Transactions. Google Scholar
Verbunt, F., Wijers, R. A. M. J., and Burm, H. M. G. 1990, Evolutionary scenarios for the x-ray binary pulsars 4U1626–67 and Her X-l and their implication for the decay of neutron star magnetic fields, Astr. Astrophys., 234, 195–202.Google Scholar
Verga, A. D. and Fontan, C. F. 1985, Soliton turbulence in a strongly magnetized plasma: Application to the coherent radio-emission of pulsars, Plasma Phys. and Controlled Fusion, 27, 19.Google Scholar
Vitarmo, J. and Jauho, P. 1973, Pulsar radio emission mechanism, Astrophys. J., 182, 935–949.Google Scholar
Vitkevitch, V. V. et al., 1976, Antenna-equipment complex BSA FIAN, Radiofizica, 19, 1594. in Russian.Google Scholar
Vivekanand, M. and Narayan, R. 1981, A new look at pulsar statistics — birthrate and evidence for injection, J. Astrophys. Astr., 2, 315–337.Google Scholar
Vivekanand, M. and Radhakrishnan, V. 1980, The structure of integrated pulse profiles, J. Astrophys. Astr., 1, 119–128.Google Scholar
Vladimirsky, B. M. 1989, Are there real types of the radiopulsars?, Astron. Zh., 30, 158.Google Scholar
Voges, W., Atmanspacher, H., and Scheingraber, H. 1987, Deterministic chaos in accreting systems: Analysis of the x-ray variability of Hercules X-l, Astrophys. J., 320, 794.Google Scholar
Volokitin, A. S., Krasnovsel'skikh, V. V., and Machabeli, G. Z. 1985, Waves in the relativistic electron-positron plasma of a pulsar, Sov. J. Plasma Phys., 11, 310.Google Scholar
Wang, D., Wu, X., and Chen, H. 1988, A possible mechanism for core emission from radio pulsars, Vistas in Astron. and Astrophys., 31, 399.Google Scholar
Webbink, R. F. 1985, Structure parameters of galactic globular clusters, in Dynamics of Star Clusters, IAU Symposium No. 113, ed. Goodman, J. and Hut, P., (Dordrecht: D. Reidel), 541–577.Google Scholar
Weekes, T. C. 1988, Very high energy gamma-ray astronomy, Phys. Reports, 160, 3.Google Scholar
Weiler, K. W. 1975, Measurement of the circular polarization in the Crab nebula at 1,415MHz, Nature, 253, 24.Google Scholar
Weisberg, J. M., Romani, R. W., and Taylor, J. H. 1989, Evidence for geodetic spin precession in the binary pulsar PSR 1913+16, Astrophys. J., 347, 1030–1033.Google Scholar
Wild, J. P., Smerd, S. F., and Weiss, A. A. 1963, Solar bursts, Ann. Rev. Astr. Ap., 1, 291.Google Scholar
Winterberg, F. 1979, Radiative collapse of relativistic electron-positron plasma to ultra-high densities, Phys. Rev., A19, 1356.Google Scholar
Wolszczan, A. 1980, A correlation of the P 3 periods of pulsars with their magnetic fields and ages, Astr. Astrophys., 86, 7–10.Google Scholar
Wolszczan, A. 1988. private communication.Google Scholar
Wolszczan, A., Anderson, S., Kulkarni, S., and Prince, T. 1989. IAU circular 4880.Google Scholar
Wolszczan, A. and Cordes, J. M. 1987, Interstellar interferometry of the pulsar PSR 1237+25, Astrophys. J., 320, L35–L39.Google Scholar
Wolszcran, A., Cordes, J. M., and Nowakowski, L. A. 1991, in preparation.Google Scholar
Wolszczan, A. and Pròszyn`ski, M. 1986, A cross-correlation analysis of subpulse drift in PSR 0809 ± 74, PSR 1237+25 and PSR 1919+21, Astrophys. J., 307, 540–544.Google Scholar
Woltjer, L. 1964, X-rays and type I supernova remnants, Astrophys. J., 140, 1309.Google Scholar
Wright, G. A. and Fowler, L. A. 1981, Mode-changing and quantized subpulse drift-rates in pulsar PSR 2319+60, Astr. Astrophys., 101, 356–361.Google Scholar
Wright, G. A., Sieber, W., and Wolszczan, A. 1986, Mode-switching, nulling and drifting subpulses in PSR 1112+50, Astr. Astrophys., 160, 402–405.Google Scholar
Wu, X. J. and Manchester, R. N. 1992, The intensity distribution of the emission beam and the discussion of radio luminosity of pulsars, in The Magnetospheric Structure and Emission Mechanisms of Radio Pulsers, IAU Colloquium No. 128, ed. Hankins, T. H., Rankin, J. M., and Gil, J. A., (Zielona Góra, Poland: Pedagogical Univ. Press), 363–366.Google Scholar
Wu, X. J., Qiao, G. J., and Xia, X. Y. 1985, The estimation of some important parameters of pulsars and the comparison between the RS model and observations, Acta Astronomica Sinica, 26, 69–75.Google Scholar
Wu, X. J., Qiao, G. J., Xia, X. Y., and Li, F. 1986, Estimation of some parameters of pulsars and their applications, Astrophys. Space Sci., 119, 101.Google Scholar
Wu, X. J., Wu, F., Deng, G. X., Qiao, G. J., and Chen, J. H. 1982, Distribution of apparent beamwidths of pulsars and evolution of their magnetic inclination, Chinese Astron. and Astrophys., 6, 216.Google Scholar
Wu, X. J., Yang, H. S., Qiao, G. J., and Deng, G. X. 1980, A statistical determination of the location of emission in pulsars based on a new classification, Chineae Astron. and Astrophys., 4, 220.Google Scholar
Wunner, G., Paez, J., Herold, H., and Ruder, H. 1986, One quantum annihilation of polarized electron-positron pairs in strong magnetic fields, Astr. Astrophys., 170, 179.Google Scholar
Xia, Y. X., Qiao, G. J., Wu, X. J., and Hou, Y. Q. 1985, Inverse Compton Scattering in strong magnetic fields and its possible application to pulsar emission, Astr. Astrophys., 152, 93.Google Scholar
Xie, R. R., Wu, X. J., Qiao, G. J., and Deng, G. X. 1985, The statistical study of emission characteristics and space distribution of the pulsars, Publication of Yunnan Astronomical Observatory, 2, 28.Google Scholar
Xilouris, K. M., Rankin, J. M., Seiradakis, J. H., and Sieber, W. 1991, Polarimetric observations of 20 weak pulsars at 1700MHz, Astr. Astrophys., 241, 87–97.Google Scholar
Yakovlev, D. G. and Urpi, V. A. 1980, Thermal and electrical conductivity in white dwarfs and neutron stars, Sov. Astron., 24, 303–310.Google Scholar
Yakovlev, D. G., Urpin, V. A., and Haensel, P. 1990, Ohmic decay in magnetized cores of neutron stars, in Proc. of Adriatic Working Party on Condensed Matter Properties of Neutron Stars, (Singapore: World Sci. Publ.)Google Scholar
Yoon, P. 1990, Amplification of a high-frequency electromagnetic wave by a relativistic plasma, Phys. Fluids, 2B, 867.Google Scholar
Yu, M. Y. and Rao, N. N. 1985, Electromagnetic pulses in a strongly magnetized electron-positron plasma, Phys. Rev., A31, 4012–4014.Google Scholar
Yu, M. Y., Shukla, P. K., and Rao, N. N. 1984, Strong electromagnetic waves in a magnetized relativistic electron-positron plasma, Astrophys. Space Sci., 107, 327.Google Scholar
Zapolsky, H. and Salpeter, E. E. 1969, The mass-radius relation for cold spheres of low mass, Astrophys. J., 158, 809.Google Scholar
Zheleznyakov, V. V. 1967, A coherent synchrotron mechanism for radio emission from cosmic sources, Soviet Phys. JETP, 24, 381.Google Scholar
Zheleznyakov, V. V., Kocharovskii, V. V., and Kocharovskii, V. V. 1989, Polarization waves and superradiance in active media, Sov. Phys. Usp., 32, 835.Google Scholar
Zheleznyakov, V. V. and Shaposhnikov, V. E. 1979, Absorption of curvature radiation, Aust. J. Phys., 32, 49.Google Scholar
Zheleznyakov, V. V. and Suvorov, E. V. 1972, Results and problems in the investigation of the synchrotron instability, Astrophys. Space Sci., 15, 24.Google Scholar
Zhu, Y. D. and Qiao, G. J. 1989, Theoretical fit for optical spectrum of the Crab pulsar, Science in China, Series A, 32, 1483.Google Scholar