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Models of Soft X-Ray Transients and Dwarf Novae

Published online by Cambridge University Press:  12 April 2016

J. P. Lasota
J. P. Lasota*
Affiliation:
UPR 176 du CNRS; DARC, Observatoire de Paris, Section de Meudon, 92190 Meudon Cedex, France

Abstract

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Models of Soft X-ray Transients are presented and compared with observations. The importance of inner advection-dominated flows in quiescent transient sources is discussed, as well as the problem of global stability of the standard outer accretion disc. A comparison is made with similar problems in dwarf nova models.

Type
X-Ray Binaries
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 385 - 394
Copyright
Copyright © Kluwer 1996

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