On the Dependence Between the Luminosities of Seyfert Galaxies and those of Their Active Nuclei

Details On the Dependence Between the Luminosities of Seyfert Galaxies and those of Their Active Nuclei On the Dependence Between the Luminosities of Seyfert Galaxies and those of Their Active Nuclei

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..468d&link_type=abstract

Astronomicheskii Zhurnal, Vol.62:3, P. 468, 1985

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Absolute magnitudes of active nuclei of some Seyfert galaxies are determined from photoelectric photometry. There exists a well-defined dependence between the luminosity (optical or bolometric) of the nucleus and the total luminosity of the parent galaxy. This is apparently not a result of observational selection only; it rather reflects a real interdependence between the nuclear activity and the properties of the galaxy as a whole. There possibly exists a sharp jump of nonstellar nuclear luminosity between normal and Seyfert galaxies.

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