No CrossRef data available.
Article contents
Outburst Phenomena in X-Ray Binaries
Published online by Cambridge University Press: 07 August 2017
Abstract
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.
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
- Copyright
- Copyright © Kluwer 1992
References
Inoue, H. (1986), Proc. IAU Symp. No.125 on
“The Origin and Evolution of Neutron Stars”, Nanjin, 1986.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
McClintock, J.E. (1990), Proc. Texas-ESO-CERN Symp. on Relativistic Astrophysics, 1990 (N.Y. Academy of Sciences).Google Scholar
Tanaka, Y. (1986), Proc. IAU Symp. No. 125 on “The Origin and Evolution of Neutron Stars”, Nanjin, 1986.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
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
You have
Access