Statistical simulations of clusters of galaxies

Details Statistical simulations of clusters of galaxies Statistical simulations of clusters of galaxies

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...209...16a&link_type=abstract

Astrophysical Journal, vol. 209, Oct. 1, 1976, pt. 1, p. 16-21

Physics

Condensed Matter

Statistical Mechanics

21

Astronomical Models, Galactic Clusters, Statistical Mechanics, Density Distribution, Distribution Functions, Error Analysis, Monte Carlo Method

Scientific paper

By comparing observed and simulated rich clusters of galaxies, it is shown that the observed clusters actually possess physical cores. The accuracy with which core radii can be determined is found. It is also shown that the observations of density profiles of galaxies in the clusters give no significant evidence for a dynamical reason as the cause of the anomalously close resemblance found previously between such density profiles and the isothermal gas distribution.

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