The neutral hydrogen deficiency of the cluster A262

Details The neutral hydrogen deficiency of the cluster A262 The neutral hydrogen deficiency of the cluster A262

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...262..442g&link_type=abstract

Astrophysical Journal, Part 1, vol. 262, Nov. 15, 1982, p. 442-450.

Astronomy and Astrophysics

Astronomy

54

Galactic Clusters, Hydrogen Clouds, Interstellar Gas, Neutral Gases, Radio Sources (Astronomy), Radio Astronomy, Red Shift, Spiral Galaxies, Tables (Data)

Scientific paper

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. 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 amouns 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.

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