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Date and Time of the Query: 2019-05-24 T04:33:13 PDT
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For refcode 1988A&AS...73..173R:
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NED Abstract

Copyright by European Southern Observatory (ESO). Reproduced by permission
1988A&AS...73..173R WSRT observations at 327 MHz of the cluster A262 G. Righetti, G. Giovannini and L. Feretti Istituto di Radioastronomia, Via Irnerio 46, I-40126 Bologna, Italy Dipartimento di Astronomia dell'Universita', Casella Postale 596, I-40100 Bologna, Italy Received August 6, accepted September 15, 1987 Summary - We present observations at 327 MHz, carried out with the WSRT in the redundancy mode, of the Abell cluster A262. The large field of view of the telescope allowed us to survey 115 CGCG galaxies, 9 of which show radio emission. A double radio source has been found to be possibly associated with NGC 679. No extended low brightness <<halo>> has been found in the cluster center. The radial distribution of radio galaxies was derived up to 100' from the cluster center. To this aim, optical plates, obtained with the Loiano telescope, were analysed to obtain accurate morphological classification and the radial distribution of galaxies. There is no evidence that the probability of producing a radio source is influenced by the position within the cluster. Key words: clusters: of galaxies - A262 - galaxies: radio.
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