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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 2.5 10(8) M., and no optical counterpart has yet been found.

The HI distribution of spiral galaxies in the cluster A 262