Accretion Disk Models with Self-Consistent Advective Cooling and Heating

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We present solutions to the accretion disk structure equations in which advective cooling is accounted for in a self-consistent way. It is shown that for high rates of accretion, above a critical value, when without advection there are no solutions extending continuously from large to small radii, there exist global solutions with self-consistent advective cooling. These solutions are quite different fromthose solutions obtained earlier by other authors, where advective cooling was not treated self-consistently.
9 pages, 4 figures, tarred and gzipped. Uses aasms4.sty

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/10297

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9601008
 http://arxiv.org/abs/astro-ph/9601008

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arXiv