On the luminosity of black hole cluster model of active galactic nuclei

Details On the luminosity of black hole cluster model of active galactic nuclei On the luminosity of black hole cluster model of active galactic nuclei

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254...61s&link_type=abstract

In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oc

Astronomy and Astrophysics

Astronomy

Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Interstellar Gas, Luminosity, Quasars, Clusters, Thermal Radiation, X Ray Sources

Scientific paper

The luminosity of a nuclear cluster of accreting black holes and other objects is discussed in terms of two accretion regimes: external supply of gas from outside the cluster and internal supply resulting from tidal disruption and capture of stars within the cluster. The external supply regime results in radiation being emitted from the innermost parts of the cluster while internal supply can efficiently feed the holes in the outer parts of the cluster as long as it is not too compact cluster and is embedded in a distribution of stars with a density larger than 10 exp 7 solar masses/cu pc.

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