Relative abundances of galaxies, intracluster gas, and dark matter in X-ray clusters of galaxies

Details Relative abundances of galaxies, intracluster gas, and dark matter in X-ray clusters of galaxies Relative abundances of galaxies, intracluster gas, and dark matter in X-ray clusters of galaxies

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pasj...44l.235f&link_type=abstract

PASJ: Publications of the Astronomical Society of Japan (ISSN 0004-6264), vol. 44, no. 6, p. L235-L240.

Astronomy and Astrophysics

Astronomy

3

Abundance, Cosmic Gases, Dark Matter, Galactic Clusters, X Ray Astronomy, Astronomical Models, Mass Distribution, Space Density

Scientific paper

We calculated self-consistently the intracluster gas distribution and its X-ray surface brightness distribution in a cluster of galaxies, while giving the mass distributions of the galaxies and dark matter. By comparing the resulting X-ray surface brightness distribution with the observational results for various clusters, we determined the relative contributions to the cluster mass densities from member galaxies, intracluster gas and dark matter, as well as their individual distributions.

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