Stability of advection-dominated accretion disks in the center of some galaxies.

Details Stability of advection-dominated accretion disks in the center of some galaxies. Stability of advection-dominated accretion disks in the center of some galaxies.

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997areps...1..178w&link_type=abstract

Astrophysics Reports, Special Issue, No. 2, p. 178 - 186

Astronomy and Astrophysics

Astrophysics

Accretion Disks: Stability, Accretion Disks: Galactic Center

Scientific paper

The local stability of advection-dominated accretion disks, which may exist in some nearby galaxies and faint AGNs, was investigated. It is found that the optically thin disk is generally more stable than the optically thick disk. This study suggests that the stable, optically thin, advection-dominated accretion disks more likely exist in the center of some inactive, less luminous galaxies.

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