The luminosity function of quasars in a merge model

Details The luminosity function of quasars in a merge model The luminosity function of quasars in a merge model

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..229k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, March 1991, p. 229-237. In Russian. In Russian.

Mathematics

Logic

2

Accretion Disks, Active Galactic Nuclei, Quasars, Spiral Galaxies, Angular Momentum, Galactic Mass, Seyfert Galaxies

Scientific paper

The luminosity function of active galactic nuclei (quasars) is
calculated within the framework of a phenomenological model. It is
assumed that the activity is governed by accretion onto a compact object
in the nucleus while accretion is due to angular momentum compensation
during the merge of spiral galaxies.

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