Galaxies-intergalactic medium interaction calculation - I. Galaxy formation as a function of large-scale environment
We present the first results of hydrodynamical simulations that follow the formation of galaxies to the present day in nearly spherical regions of radius ~20h-1Mpc drawn from the Millennium Simulation (Springel et al.). The regions have mean overdensities that deviate by (-2, -1, 0, +1, +2)σ from the cosmic mean, where σ is the rms mass fluctuation
Crain, Robert A. et al.
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2009