The asymmetry of the Coma cluster of galaxies

Details The asymmetry of the Coma cluster of galaxies The asymmetry of the Coma cluster of galaxies

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990an....311...89b&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 311, no. 2, 1990, p. 89-97.

Astronomy and Astrophysics

Astronomy

16

Asymmetry, Galactic Clusters, Galactic Radiation, Galactic Structure, Radial Velocity, Radio Astronomy, Space Density, X Ray Astronomy

Scientific paper

A detailed reinvestigation of the Coma cluster basing on enlarged observational material of number density distributions and radial velocities of galaxies as well as radio and X-ray data is performed and supports our previous conclusion that this cluster possesses a substructure. This substructure is in the south-western region of the cluster and produces the impression of an elongated cluster structure in the direction of the bridge between Coma and A 1367. A 1656 seems to be a cD-like cluster with NGC 4874 as the only dominating giant central galaxy.

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