Accretion Disks in Transient Systems

Details Accretion Disks in Transient Systems Accretion Disks in Transient Systems

1997-12-15

arxiv.org/abs/astro-ph/9712185v1

Astronomy and Astrophysics

Astrophysics

16 pages, 0 figures

Scientific paper

I review recent advances in our understanding of accretion disks in transient systems - the dwarf novae and the soft X-ray transients. The primary theme will be the ongoing development of theory in response to the observations. The accretion disk limit cycle model appears to provide a unifying framework within which we may begin to understand what is seen in different types of interacting binary stars, and also to constrain parameters which enter into the theory.

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