Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-29T15:41:39.877Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsars and their Genesis

Published online by Cambridge University Press:  30 March 2016

V. Radhakrishnan
V. Radhakrishnan*
Affiliation:
Raman Research Institute, Bangalore 560 080, India

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The subject I have chosen for my talk today will come of age on the last day of this General Assembly. The first detection of the remarkable objects that we call pulsars, was on 28th November 1967 when Jocelyn Bell (now Bell-Burnell) who was working with Prof. Hewish at Cambridge discovered a new class of radio sources that put out pulses of radio radiation about once a second but with clock-like regularity. Two other major discoveries in the same decade using the radio spectrum were, of course, Quasars and the Cosmic microwave background. Those two took us to extremes in time and distance, and the amount of energy radiated, whereas the discovery of pulsars, situated near at hand by comparison, led us to extremes in the physical state of matter.

Type
Invited Discourses
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 3 - 26
Copyright
Copyright © Reidel 1986

References

Anderson, B. and Lyne, A.G. 1983, Nature 303, 597.CrossRefGoogle Scholar
Baade, W. and Zwicky, F. 1934, Proc. Nat. Acad. Sci. (U.S.A.) 20, 254.Google Scholar
Backer, D.C., Kulkarni, S.R., Heiles, C., Davis, M.M. and Goss, W.M. 1982, Nature 300, 615.CrossRefGoogle Scholar
Boriakoff, V., Buccheri, R. and Fauci, F. 1983, Nature 304, 417.CrossRefGoogle Scholar
Chevalier, R.A. and Emmering, R.T. 1985, (to appear in Astrophys. J.).Google Scholar
Cordes, J.M. and Weisberg, J.M. 1984, in Millisecond Pulsars, eds. Reynolds, S.P. & Stinebring, D.R. (NRAO, Green Bank, W.Va., U.S.A.), p.138.Google Scholar
Davidson, K. and Ostriker, J.P. 1973, Astrophys. J. 179, 583.Google Scholar
Davis, M., Taylor, J., Weisberg, J. and Backer, D. 1984, in Millisecond Pulsars, eds. Reynolds, S.P. & stinebring, D.R. (NRAO, Green Bank, W.Va., U.S.A.), p.12.Google Scholar
Giacconi, R., Gursky, H., Paolini, F.R. and Rossi, B.R. 1962, Phys. Rev. Lett. 9, 439.Google Scholar
Ginzburg, V.L. 1971, in Highlights of Astronomy, Vol. 2, ed. Jager, C. de. (Reidel, Dordrecht) p.20.CrossRefGoogle Scholar
Goldreich, P. 1972, in The Physics of Pulsars, ed. Lenchek, A.M. (Gordon & Breach, New York), p.151.Google Scholar
Green, D.A., and Gull, S.F. 1983, in IAU Symp. 101: Supernova Remnants and Their X-ray Emission, eds. Danziger, J. & Gorenstein, P. (Reidel, Dordrecht), p.329.CrossRefGoogle Scholar
Gunn, J.E. and Ostriker, J.P. 1970, Astrophys. J. 160, 979.Google Scholar
Hewish, A., 1971, in Highlights of Astronomy, Vol. 2, ed. Jager, C. de. (Reidel, Dordrecht), p.18.Google Scholar
Hewish, A., Bell, S.J., Pilkington, J.D.H., Scott, P.F. and Collins, R.A. 1968, Nature 217, 709.Google Scholar
Hulse, R.A. and Taylor, J.H. 1974, Astrophys.J.(Lett.) 191, L59.CrossRefGoogle Scholar
Iben, I. and Tutukov, A.V. 1985, Astrophys.J. Supp. 58, 661.Google Scholar
Large, M.I., Vaughan, A.E. and Mills, B.Y. 1968, Nature 220, 340.Google Scholar
Lyne, A.G., Anderson, B. and Salter, M.J. 1982, Mon. Not. R. Astr. Soc. 201, 503.CrossRefGoogle Scholar
Narayan, R. and Vivekanand, M. 1983, Astron. Astrophys. 122, 45.Google Scholar
Manchester, R.N. and Taylor, J.H. 1977, “Pulsars” (W.H. Freeman, San Francisco).Google Scholar
Miller, J.S. and Wampler, E.J. 1969, Nature 221, 1037.CrossRefGoogle Scholar
Murray, S.S., Fabbiano, G., Fabian, A.C., Epstein, A. and Giacconi, R. 1979, Astrophys.J. 234, L69.CrossRefGoogle Scholar
Oppenheimer, J.R. and Volkoff, G.M. 1939, Phys. Rev. 55, 374.Google Scholar
Ostriker, J.P. and Gunn, J.E. 1969, Astrophys.J. 157, 1395.CrossRefGoogle Scholar
Paczynski, B. 1971, Ann. Rev. Astr. Astrophys. 9, 183.Google Scholar
Pringle, J.E. and Rees, M.J. 1972, Astron. Astrophys. 21, 1.Google Scholar
Proszynski, M. and Przybycien, D. 1984, in Millisecond Pulsars, eds. Reynolds, S.P. & stinebring, D.R. (NRAO, Green Bank, W.Va., U.S.A.), p.151.Google Scholar
Radhakrishnan, V. 1984, in Proceedings of Millisecond Pulsars, eds. Reynolds, S.P. & Stinebring, D.R. (NRAO, Green Bank, W.Va., U.S.A.), p.130.Google Scholar
Radhakrishnan, V., Cooke, D.J., Komesaroff, M.M. and Morris, D. 1969, Nature 221, 443.Google Scholar
Radhakrishnan, V. and Cooke, D.J. 1969, Astrophys.Lett. 3, 225.Google Scholar
Radhakrishnan, V. and Srinivasan, G. 1982, Curr. Sci. 51, 1096.Google Scholar
Radhakrishnan, V. and Srinivasan, G. 1984, in the Proceedings of the Second Asian-Pacific Regional Meeting on Astronomy, eds. Hidayat, B. & Feast, M.W. (Tira Pustaka, Jakarta, Indonesia), p. 423.Google Scholar
Radhakrishnan, V. and Shukre, C.S. 1985, in the Proceedings of the workshop on Supernovae, their Progenitors and Remnants, eds. Srinivasan, G. & Radhakrishnan, V. (Indian Acad. Sci., Bangalore, India), p.155.Google Scholar
Richards, D.W. and Cornelia, J.M. 1969, Nature 222, 551.CrossRefGoogle Scholar
Ruderman, M. 1981, in IAU Symp. 95: Pulsars, eds. Sieber, W. & Wielebinski, R., (Reidel, Dordrecht), p.87.Google Scholar
Ruderman, M. 1986, in Proceedings of the NATO Advanced Study Institute on “High Energy Phenomena Around Collapsed Stars”, Cargese, Sept. 1985.Google Scholar
Shklovsky, I.S. 1968, Sov. Astron. 11, 749.Google Scholar
Smarr, L.L. and Blandford, R. 1976, Astrophys.J. 207, 574.Google Scholar
Srinivasan, G. and van den Heuvel, E.P.J. 1982, Astron. Astrophys. 108, 143.Google Scholar
Srinivasan, G., Bhattacharya, D. and Dwarakanath, K.S. 1984, J. Astrophys. Astron. 5, 403.Google Scholar
Staelin, D.H. and Reifenstein, E.C. 1968, Science 162, 1481.Google Scholar
Stokes, G.H., Taylor, J.H. and Dewey, R.J. 1985, Astrophys.J. (Lett.) 294, L.21.Google Scholar
Stokes, G.H., Taylor, J.H., Weisberg, J.M. and Dewey, R.J. 1985, Nature 317, 787.Google Scholar
Sturrock, P.A. 1971, Astrophys.J. 164, 529.CrossRefGoogle Scholar
Taylor, J.H. and Weisberg, J. 1982, Astrophys.J. 233, 908.CrossRefGoogle Scholar
Tutukov, A.V. 1981, in IAU Symp. 93: Fundamental Problems in the Theory of Stellar Evolutions, eds. Sugimoto, D., Lamb, D.Q. & Schramm, D.N. (Reidel, Dordrecht), p.137.Google Scholar
van den Heuvel, E.P.J. 1981, in IAU Symp. 93: Fundamental Problems in the Theory of Stellar Evolution, Eds. Sugimoto, D., Lamb, D.Q. & Schramm, D.N. (Reidel, Dordrecht), p.155.Google Scholar
van den Heuvel, E.P.J. 1983, in Accretion Driven Stellar X-ray Sources, in eds. Lewin, W.H.G. & van den Heuvel, E.P.J (Cambridge Univ. Press.), p.303.Google Scholar
van den Heuvel, E.P.J., and Bonsema, P.T.J. 1984, Astron. Astrophys. 139, L.16.Google Scholar
van der Klis, M., Jansen, F., van Paradijs, J., Lewin, W.H.G., van den Heuvel, E.P.J., Trumper, J.E. and Sztajno, M. 1985, Nature 316, 225.CrossRefGoogle Scholar
Vivekanand, M. and Narayan, R. 1981, J. Astrophys. Astron. 2, 315.Google Scholar
Vivekanand, M., Narayan, R. and Radhakrishnan, V. 1982, J. Astrophys. Astron. 3, 237.CrossRefGoogle Scholar
Vivekanand, M. and Narayan, R. 1982, J. Astrophys. Astron. 3, 399.Google Scholar
Zeldovich, Ya.B. 1964, Sov. Phys. Doklady 9, 246.Google Scholar