Models of Soft X-Ray Transients and Dwarf Novae

Details Models of Soft X-Ray Transients and Dwarf Novae Models of Soft X-Ray Transients and Dwarf Novae

1995-09-01

arxiv.org/abs/astro-ph/9509003v1

Astrophys.Space Sci.Libr. 208 (1996) 385

Astronomy and Astrophysics

Astrophysics

10 pages, 3 figures (available as uuencoded compressed tar file). Invited review at IAU Colloquium 158 "Cataclysmic Variables

Scientific paper

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.

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