The 102.5-MHz emission of Abell clusters with Z = 0.02-0.075. III - Local radio luminosity function

Details The 102.5-MHz emission of Abell clusters with Z = 0.02-0.075. III - Local radio luminosity function The 102.5-MHz emission of Abell clusters with Z = 0.02-0.075. III - Local radio luminosity function

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63....1g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, Jan.-Feb. 1986, p. 1-15) Soviet Astronomy (ISSN 0038-5301), vol. 30, Jan.-Feb. 1986, p. 1-10

Statistics

Computation

3

Emission Spectra, Functions (Mathematics), Galactic Clusters, Luminosity, Radio Spectra, Computational Astrophysics, Mass Distribution, Radio Frequencies, Red Shift

Scientific paper

The local radio luminosity function of Abell clusters of galaxies is constructed at 102.5 MHz from ≡1024 to ≡1027W Hz-1 and for total radio luminosities from ≡1040 to ≡1043erg s-1. The behaviour of the clusters' radio luminosity function agrees well with the known properties of the radio luminosity function of galaxies.

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