The mass-luminosity relation for active galactic nuclei

Details The mass-luminosity relation for active galactic nuclei The mass-luminosity relation for active galactic nuclei

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..283r&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Oct. 1987, p. 283-293. In Russian.

Astronomy and Astrophysics

Astronomy

4

Active Galactic Nuclei, Astronomical Catalogs, Luminous Intensity, Stellar Mass, Infrared Astronomy, Mass To Light Ratios, Quasars, Seyfert Galaxies, Spectral Bands

Scientific paper

The paper deals with the dependence of the active nuclei luminosity in
various spectral bands on their mass based on the Catalogue of data for
active galactic nuclei by E. A. Dibaj. It has been shown that for
Seyfert 1 galaxies and nearby quasars Lbol ≡
m4/3 satisfies Hill's model.

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