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The neutral hydrogen deficiency of the cluster A262

Seventy-two galaxies in the spiral-rich cluster A262 have been observed in the 21 cm line at Arecibo of which 67 have been observed by us. The H I content of individual galaxies, as compared with that of a sample of isolated galaxies, depends on the distance from the core of the cluster; while pronounced H I deficiency is observed near the central parts, normal amounts of H I are observed in the cluster periphery. With the newly available redshifts, a revised set of dynamical parameters for the cluster are given.