The kinematics and dynamics of the rich cluster of galaxies Abell 539

Details The kinematics and dynamics of the rich cluster of galaxies Abell 539 The kinematics and dynamics of the rich cluster of galaxies Abell 539

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....96.1775o&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 96, Dec. 1988, p. 1775-1790. Research supported by Harvard University.

Astronomy and Astrophysics

Astronomy

47

Astronomical Photometry, Astronomical Spectroscopy, Galactic Clusters, X Ray Sources, Charge Coupled Devices, Luminosity, Mass To Light Ratios, Radial Velocity, Velocity Distribution

Scientific paper

A sample of 289 redshifts within 10 deg of the center of the cluster A539 have been obtained in order to investigate the cluster kinematics and dynamics. Within 1 Mpc of the center, the physical parameters of A539 are found to be typical of those of rich clusters. It is shown that early-type galaxies are more concentrated toward the cluster center and that the velocity distributions of early-type and late-type galaxies differ marginally.

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