Thermal equilibria of accretion disks
Sep, 1994
8 pages
Published in:
- Astrophys.J.Lett. 438 (1995) L37
e-Print:
- astro-ph/9409018 [astro-ph]
DOI:
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Abstract: (arXiv)
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.References(2)
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