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Radio Properties of Abell Clusters

Published online by Cambridge University Press:  14 August 2015

C. Lari  and
G.C. Perola
C. Lari
Affiliation:
Laboratorio di Radioastronomia, Bologna
G.C. Perola
Affiliation:
Istituto di Scienze Fisiche dell'Università, Milano

Extract

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Since the early 60's the association of some radio sources with rich clusters of galaxies was noted (Mills, 1960; van den Bergh, 1961) and subsequent investigations concentrated mostly on the radio properties of clusters in the Abell catalogue. This paper is confined to this subject, although one should bear in mind the importance of associations with other scales of clustering which do not appear as entries of that catalogue. in this paper we shall use HO = 100 km sec−1 and the radio power P in WHz−1 at 408 MHz.

Information

Type
II. Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 137 - 147
Copyright
Copyright © Reidel 1978 

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