Astronomy and Astrophysics – Astrophysics
Scientific paper
1994-09-09
Astrophys.J. 438 (1995) L37
Astronomy and Astrophysics
Astrophysics
Submitted to ApJL July 1994. PS file, 8 Pages; 3 Figs available upon request
Scientific paper
10.1086/187709
We show that most of hot, optically thin accretion disk models which ignore
advective cooling are not self-consistent. We have found new types of optically
thin disk solutions where cooling is dominated by radial advection of heat.
These new solutions are thermally and viscously stable.
Abramowicz Marek A.
Chen Xingming
Kato Shoji
Lasota Jean-Pierre
Regev Oded
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