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SIMULATION OF AN INDIVIDUAL CLUSTER
AN OVERVIEW OF THE CLUSTER ENSEMBLE
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2F run abundance gradient baryon fraction best fit binding mass cluster galaxies cluster gas cluster mass comoving coordinates core radius correlation cosmological curves dark matter density dynamical friction effect ejection ensemble ejection runs Equation Evrard EXOSAT expected feedback Figure fluid galactic winds galaxy clusters galaxy number density gas density profile gas particle gas temperature gravitational high redshift hydrostatic hydrostatic equation hydrostatic equilibrium infall intracluster gas intracluster medium iron abundance profile isothermal logarithmic slope luminosity function mass estimates mass scale matter density profile mean interior merger metallicity number density profile observations perturbation potential power law power spectrum predicted radial radii ratio real clusters redshift relation result rich clusters ROSAT run with ejection sample run shown shows simulated clusters specific energy steeper surface brightness surface brightness profiles thermal timestep two-fluid ensemble two-fluid runs typically universe velocity bias velocity dispersion virial radius X-ray surface brightness