Simulating the interaction of galaxies and the intergalactic medium
The co-evolution of galaxies and the intergalactic medium as a function of environment is studied using hydrodynamic simulations of the ACDM cosmogony. It is demonstrated with non-radiative calculations that, in the absence of non-gravitational mechanisms, dark matter haloes accrete a near-universal...
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Durham University
2008
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.549963 |