102. 5-MHz emission of Abell clusters with z = 0. 02-0. 075. III. Local radio luminosity function

Journal Article · Sat Feb 01 04:00:00 EST 1986 · Sov. Astron. (Engl. Transl.); (United States)

OSTI ID:6689465

Gubanov, A G

A local radio luminosity function (RLF) is derived for Abell clusters of galaxies, extending from about (1-1000) x 10 to the 24th W/Hz at 102.5-MHz frequency, or about (1-1000) x 10 to the 40th erg/s integrated over all radio frequencies. The behavior of this cluster RLF is consistent with properties previously established for galaxy RLFs. 29 references.

• Research Organization: Leningradskii Gosudarstvennyi Universitet, Leningrad, USSR
• OSTI ID: 6689465
• Journal Information: Sov. Astron. (Engl. Transl.); (United States), Journal Name: Sov. Astron. (Engl. Transl.); (United States) Vol. 30; ISSN SAAJA
• Country of Publication: United States
• Language: English

Related Subjects

640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
DISTRIBUTION
ELECTROMAGNETIC RADIATION
EMISSION SPECTRA
GALAXY CLUSTERS
LUMINOSITY
MASS DISTRIBUTION
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
RADIATIONS
RADIOWAVE RADIATION
RED SHIFT
SPATIAL DISTRIBUTION
SPECTRA