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Outburst Phenomena in X-Ray Binaries

Published online by Cambridge University Press:  07 August 2017

Y. Tanaka
Y. Tanaka*
Affiliation:
Institute of Space and Astronautical Science 3-1-1 Yoshinodai, Sagamihara, Kanagawa-ken 229, Japan

Abstract

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Three distinctly different types of outburst phenomenon in X-ray binaries are discussed: (1) the so-called type 1 burst which is a thermonuclear flash of matter accreted on the surface of neutron stars, (2) the so-called type 2 burst which is a burst-like X-ray emission caused by a spasmodic accretion, and (3) the nova-like outburst which is triggered by a sudden commencement of accretion.

Type
Invited Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 215 - 224
Copyright
Copyright © Kluwer 1992 

References

Baym, G. and Pethick, C. (1979), Ann. Rev. Astron. Astrophys., 17, 415.Google Scholar
Ebisuzaki, T. (1987), Publ. Astron. Soc. Japan, 39, 287.Google Scholar
Elvis, M. et al. ((1975), Nature, 257, 656.Google Scholar
Inoue, H. et al. (1984), Publ. Astron. Soc. Japan, 36, 831.Google Scholar
Inoue, H. (1986), Proc. IAU Symp. No.125 on “The Origin and Evolution of Neutron Stars”, Nanjin, 1986.Google Scholar
Kaluzienski, L.J. et al. (1977), Astrophys. J., 212, 203.Google Scholar
Kitamoto, S. et al. (1990), Astrophys. J., 361, 590.Google Scholar
Lewin, W.H.G. and Joss, P.C. (1983), Accretion-Driven Stellar X-Ray Sources, eds. Lewin, W.H.G. and van den Heuvel, E.P.J. (Cambridge University Press), p41.Google Scholar
London, R.A., Taam, R.E. and Howard, W.M. (1986), Astrophys. J. 306, 142.Google Scholar
Lund, N. and Brandt, S. (1991), IAU Circular 5161.Google Scholar
Magnier, E. et al. (1989), M.N.R.A.S., 237, 729.Google Scholar
Makino, F. (1989), IAU Circular 4782, and IAU Circular 5161.Google Scholar
McClintock, J.E. (1990), Proc. Texas-ESO-CERN Symp. on Relativistic Astrophysics, 1990 (N.Y. Academy of Sciences).Google Scholar
Nagase, F. (1989), Publ. Astron. Soc. Japan, 41, 1.Google Scholar
Nagase, F. (1989), Proc. 23rd. ESLAB Symp. (ESA SP-296), p45.Google Scholar
Nakamura, N., Inoue, H. and Tanaka, Y. (1988), Publ. Astron. Soc. Japan, 40, 209.Google Scholar
Tanaka, Y. (1986), Proc. IAU Symp. No. 125 on “The Origin and Evolution of Neutron Stars”, Nanjin, 1986.Google Scholar
Tanaka, Y. (1989), Proc. 23rd. ESLAB Symp. (ESA Sp-296), p3.Google Scholar
Tanaka, Y. (1991), Proc. Symp. on “X-Ray Binaries and the Formation of Binary and Millisecond Radio Pulsars”, Santa Barbara, 1991.Google Scholar
Tawara, Y. et al. (1985), Nature, 318, 545.CrossRefGoogle Scholar
Tsunemi, H. et al. (1989), Astrophys. J. Letters, 337, L81.Google Scholar
Waki, I, et al. (1984), Publ. Astron. Soc. Japan, 36, 819.Google Scholar
White, N.E., Kaluzienski, J.L. and Swank, J.H. (1984), High Energy Transients in Astrophysics, ed. Woosley, S.E. (N. Y.: AIP), p31.Google Scholar