Redshifts of galaxies in the cluster Abell 262, and in the region of the Pisces group /centred on NGC 383/

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Elliptical Galaxies, Galactic Clusters, Radial Velocity, Red Shift, Spiral Galaxies, Astronomical Spectroscopy, Galactic Nuclei, Galactic Structure, Luminous Intensity, Velocity Distribution

Scientific paper

Redshifts are presented for galaxies in the Abell 262 cluster and for galaxies within approximately 2 deg on the sky of the Pisces group, otherwise known as the chain of galaxies centered on NGC 383. Mean redshifts and corrected velocity dipersions are determined for both groupings, the distribution of bright galaxies in Abell 262 is shown to exhibit a flattened structure, and the problem of distinguishing cluster members from nonmembers is examined. Velocity distributions are compared for the Virgo, Abell 1367, Abell 262, Abell 194, and Centaurus clusters. A model of cluster formation involving the collapse of an expanding initial bound perturbation is considered, and virial-mass determination is discussed.

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