Studying high redshift galaxy clusters with the ESO Distant Cluster Survey

Details Studying high redshift galaxy clusters with the ESO Distant Cluster Survey Studying high redshift galaxy clusters with the ESO Distant Cluster Survey

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003msngr.112...19r&link_type=abstract

The Messenger (ISSN 0722-6691), No. 112, p. 19 - 24 (June 2003)

Mathematics

Logic

3

Galaxy Clusters, Redshifts, Surveys

Scientific paper

Galaxy clusters are the most massive quasi-equilibrium objects in the Universe and are the meeting places of the cosmos. Their deep potential wells are dominated by unseen dark matter, but contain a cosmologically representative baryon fraction in the form of galaxies and intergalactic gas. These are trapped in a virialized state, with the gas heated to tens of millions of degrees and the galaxies moving with rms velocities of ~1000 km/s.

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