Published March 1984
| Version v1
Journal article
Thermal convection in black hole accretion disks
Creators
- 1. Abastumani Astrophysical Observatory, Georgian Academy of Sciences
Description
A linear theory is developed for thermal convective instability in radiating gas dominated by radiation pressure. Analysis demonstrates how the magnetic field and differential rotation will affect the onset of thermal convection in the interior of a black hole accretion disk
Additional details
Publishing Information
- Journal Title
- Sov. Astron. (Engl. Transl.)
- Journal Volume
- 28
- Journal Issue
- 2
- Series
- Sov. Astron. (Engl. Transl.).
- Journal Page Range
- 168-172
- ISSN
- 0038-5301
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 16025624
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCRETION DISKS; BLACK HOLES; CONVECTION; CONVECTIVE INSTABILITIES; MAGNETIC FIELDS; RADIATION PRESSURE; ROTATION
- Descriptors DEC
- ENERGY TRANSFER; HEAT TRANSFER; INSTABILITY; PLASMA INSTABILITY
Optional Information
- Notes
- Cover-to-cover translation of Astronomicheskij Zhurnal (USSR).