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Thermal equilibria of accretion disks
Open accessAbstract
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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Citations
Cited by
Hot Accretion Flows Around Black Holes
Yuan, F., & Narayan, R. (2014) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-082812-141003 · Cited by 1,529
On the fate of gas accreting at a low rate on to a black hole
Blandford, R. D., & Begelman, M. C. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02358.x · Cited by 1,439
Esin, A. A., McClintock, J. E., & Narayan, R. (1997) · The Astrophysical Journal · doi:10.1086/304829 · Cited by 1,313
THE GALACTIC CENTER ENVIRONMENT
Morris, M., & Serabyn, E. (1996) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.34.1.645 · Cited by 930
McKinney, J. C., Tchekhovskoy, A., & Blandford, R. D. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21074.x · Cited by 931
Metadata
- Authors
- Abramowicz, M. A., Chen, X., Kato, S., Lasota, J.-P., & Regev, O.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1995-01
- Volume
- 438
- Pages
- L37
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2057386138
- Cited by
- 602
- References
- 0
- FWCI
- 22.85
- Type
- journal article
- Language
- en
- Open access
- green
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- Abramowicz, M. A., Chen, X., Kato, S., Lasota, J.-P., & Regev, O. (1995). Thermal equilibria of accretion disks. The Astrophysical Journal. https://doi.org/10.1086/187709
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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