Evolution of radio quasars for Z of less than 2

Details Evolution of radio quasars for Z of less than 2 Evolution of radio quasars for Z of less than 2

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97.1291n&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, May 1989, p. 1291-1305.

Astronomy and Astrophysics

Astronomy

35

Evolution (Development), Quasars, Luminosity, Red Shift, Spatial Distribution, Very Large Array (Vla)

Scientific paper

A sample of 72 radio quasars is used to study the cosmic and individual evolution of quasars in the 1-2 redshift range. It is shown that the most luminous sources at all redshifts are unresolved, and that one-sided and two-sided structures correspond to progressively lower core (and total) luminosities. The sizes and fractional population of triple sources are found to fall steadily with increasing redshift to z of about 1.7. A correlation over many orders of magnitude is noted between the optical and maximum radio-core luminosity.

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