Thermal equilibria of accretion disks

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 1995Embargo end date: 01 Jan 1994 English Publisher:American Astronomical SocietyJournal:The Astrophysical Journal, volume 438, page L37 (issn: 0004-637X, eissn: 1538-4357,

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Authors: Abramowicz, Marek A.; Chen, Xingming; Kato, Shoji; Lasota, Jean-Pierre; Regev, Oded;

doi: 10.1086/187709 , 10.48550/arxiv.astro-ph/9409018

arXiv: astro-ph/9409018

Thermal equilibria of accretion disks

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Abstract

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.

Submitted to ApJL July 1994. PS file, 8 Pages; 3 Figs available upon request

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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