From local active galactic nuclei to early quasars

Details From local active galactic nuclei to early quasars From local active galactic nuclei to early quasars

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...296..402c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 296, Sept. 15, 1985, p. 402-415. Research supported by the Ministero della

Mathematics

37

Active Galactic Nuclei, Astronomical Models, Luminosity, Quasars, Cosmology, Functions (Mathematics)

Scientific paper

To close the gap between the local luminosity function of the optically selected active galactic nuclei and the population properties of distant (z less than about 2) quasars, a model of differential luminosity evolution is proposed, which is astrophysically based and contains a minimal number of free parameters. The advantages of the model and its predictions are discussed, and how to extend it for z greater than 2 to cover the beginning of the quasar era, is indicated.

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