Accretion Disk Models with Self-Consistent Advective Cooling and Heating

Details Accretion Disk Models with Self-Consistent Advective Cooling and Heating Accretion Disk Models with Self-Consistent Advective Cooling and Heating

1996-01-03

arxiv.org/abs/astro-ph/9601008v1

Astronomy and Astrophysics

Astrophysics

9 pages, 4 figures, tarred and gzipped. Uses aasms4.sty

Scientific paper

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.

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