The structure and dynamics of rich clusters of galaxies.

Details The structure and dynamics of rich clusters of galaxies. The structure and dynamics of rich clusters of galaxies.

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989msngr..57...30m&link_type=abstract

The Messenger, vol. 57, p. 30-32

Computer Science

3

Clusters Of Galaxies: Dynamics, Clusters Of Galaxies: Structure

Scientific paper

Rich clusters of galaxies are of great interest for several reasons. As the largest bound structures that can be fairly easily found and studied in detail, they represent a formidable constraint for theories of the formation of largescale structure in the Universe. In addition, they provide an ideal laboratory for the study of the behaviour of galaxies in an environment of high galaxy-density; quite frequently in the presence of a hot, X-ray emitting, intracluster gas, that may have a mass comparable to the total visible mass in galaxies. As rich clusters can be detected out to fairly high redshifts, they also allow one to study the evolution of the galaxy population in clusters over an appreciable fraction of the Hubble time. Even the evolution of their global structure on such timescales is amenable to study (Gunn, 1989).

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