Accretion Disk Models with Self-Consistent Advective Cooling and Heating
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/9601008,
title = {Accretion Disk Models with Self-Consistent Advective Cooling and Heating},
author = {I. V. Artemova and G. S. Bisnovatyi-Kogan and G. Bjornsson and I. Novikov},
journal= {arXiv preprint arXiv:astro-ph/9601008},
year = {2007}
}
Comments
9 pages, 4 figures, tarred and gzipped. Uses aasms4.sty