Properties of cluster satellites in hydrodynamical simulations
Properties of cluster satellites in hydrodynamical simulations
We analyse the dynamical and thermal evolution of dark matter and the intracluster medium in hydrodynamical N-body simulations of galaxy clusters. Starting from a sample of 17 high-resolution objects, with virial mass ranging from 3 × 1014 to 1.7 × 1015h−1 M⊙, we follow the build-up of the systems in …