Year: 1995
Type: article
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.
Source: The Astrophysical Journal
DOI: 10.1086/187709
Authors: Marek A. Abramowicz, Xingming Chen, Shoji Kato, Jean-Pierre Lasota, Oded Regev
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2057386138