The Role Of Intra-Cluster Gas In Dynamical Evolution Of The Galaxy Cluster Embedded In The Dark Matter Halo

Physics – High Energy Physics

Scientific paper

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Clusters Of Galaxies, Dark Matter, Brightness, X-Ray Emission Spectra, Galaxy Clusters, Dark Matter, Magnitudes And Colors, Luminosities, X-Ray Binaries

Scientific paper

Numerical simulations of dynamic evolution of the cluster consisting of 1000 galaxies, 6000 hypothetical «grains» of Dark Matter (DM) and Intra-Cluster-gas (IC-gas) have been performed in the framework of N-body problem to clarify roles of these components in formation of a cD-galaxy. Analysis of simulation results shows the low efficiency of tidal braking produced by DM, the high efficiency of the IC-gas ram pressure stripping internal galaxy's gas and importance of realistic gas model choice.

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