Analysis of density profiles of clusters of galaxies.

Details Analysis of density profiles of clusters of galaxies. Analysis of density profiles of clusters of galaxies.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..597l&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 597 - 598

Astronomy and Astrophysics

Astrophysics

Clusters Of Galaxies: Densities

Scientific paper

The authors perform a statistical analysis of the galaxy density profiles of clusters of galaxies. They consider all clusters of galaxies with published redshifts z < 0.12 in the area covered by the COSMOS/UKST Southern Sky Galaxy Catalogue. The results of the statistical analysis indicate that a single power-law model provides a very good fit to the data. Cluster density profiles are found consistent with an isothermal model with a weak tendency toward flatter profiles for richer objects.

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