The Ursa Major supercluster. II - A statistical analysis of the radio survey

Details The Ursa Major supercluster. II - A statistical analysis of the radio survey The Ursa Major supercluster. II - A statistical analysis of the radio survey

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204.1245s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Sept. 1983, p. 1245-1256. Research supported by th

Astronomy and Astrophysics

Astronomy

4

Galactic Clusters, Radio Galaxies, Statistical Analysis, Astronomical Catalogs, Indexes, Luminous Intensity, Statistical Distributions

Scientific paper

A statistical analysis of the 5C 10 radio survey of the Ursa Major supercluster is used to derive estimates for the radio luminosity distribution of the central cluster (Abell 1318) and the whole supercluster. Galaxies within the supercluster only form about 12 per cent of the total number of radio sources, and only 3 per cent of the galaxies were detected. The overall radio source counts and spectral-index distribution are compatible with previous 5C surveys, but there is a significant difference between the spectral-index distribution and that found for more intense sources. This difference has implications for the radio source counts.

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