Thermal Equilibria of Accretion Disks

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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