NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-05-27 T02:01:31 PDT
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For refcode 1997A&AS..126..537B:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
1997A&AS..126..537B The HI distribution of spiral galaxies in the cluster A 262. Bravo-Alfaro H., Szomoru A., Cayatte V., Balkowski C., Sancisi R. Received October 31, 1996; accepted April 21, 1997 Abstract. We present results of an Hi survey of the cluster of galaxies Abell 262, using the Westerbork Synthesis Radio Telescope (WSRT). Eleven galaxies were detected in five fields. In a few cases the gas in these galaxies shows an asymmetrical distribution; the most likely explanation is the interaction between the cluster medium and the gaseous disks. Only two of the detected galaxies are slightly Hi-deficient. At 40" to the West of CGCG 160-049 we tentatively detect what may be an associated Hi cloud. The total mass of this cloud is 2.5x10^8^M_sun_, and no optical counterpart has yet been found. Key words: galaxies: clusters: individual: Abell 262 - radio lines: galaxies
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