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Hydrodynamic Models of Line-Driven Accretion Disk Winds in Cataclysmic Variables

We developed several alpha-disk models for line-driven winds from cataclysmi c variables. Using 1-D analytic models we explore the conditions necessary for th e existence of a wind, and the dependence of speed and mass-loss with radius. Using a 2-D isothermal model we explore the effects of centrifu...

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Publicat a:Revista Mexicana de Astronomía y Astrofísica
Autors principals: Nicolas Antonio Pereyra, Timothy R. Kallman, John M. Blondin
Format: Artigo
Idioma:Inglês
Publicat: Universidad Nacional Autónoma de México 2001
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Accés en línia:https://www.redalyc.org/articulo.oa?id=57101150
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