Accretion Disks in Transient Systems

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dc.creatorCannizzo, John K.
dc.date1997-12-15
dc.date.accessioned2026-07-07T02:25:35Z
dc.date.available2026-07-07T02:25:35Z
dc.descriptionI 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.
dc.description16 pages, 0 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9712185
dc.identifierhttp://arxiv.org/abs/astro-ph/9712185
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11934
dc.subjectAstrophysics
dc.titleAccretion Disks in Transient Systems
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