Estimates of a nuclear luminosity function of Seyfert galaxies

Details Estimates of a nuclear luminosity function of Seyfert galaxies Estimates of a nuclear luminosity function of Seyfert galaxies

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.140..353m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 140, no. 2, Jan. 1988, p. 353-358.

Astronomy and Astrophysics

Astrophysics

1

Active Galactic Nuclei, Luminous Intensity, Quasars, Seyfert Galaxies, Error Analysis, Space Density

Scientific paper

Nuclear magnitudes of Seyfert galaxies, determined from two-dimensional photometric data, are used to make an estimate of the luminosity function (LF) of Seyfert nuclei. This provides a direct observational check of two indirect determinations of this LF, one of which is favoured by the present result. Comparisons with the Seyfert LF for integrated magnitudes, the local quasar LF, and the LF of field galaxies, are discussed.

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