Models of Soft X-Ray Transients and Dwarf Novae
Astrophysics
2016-01-27 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/9509003,
title = {Models of Soft X-Ray Transients and Dwarf Novae},
author = {J. P. Lasota},
journal= {arXiv preprint arXiv:astro-ph/9509003},
year = {2016}
}
Comments
10 pages, 3 figures (available as uuencoded compressed tar file). Invited review at IAU Colloquium 158 "Cataclysmic Variables and Related Objects", Keele. 26-30 June 1995