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Comparing the temperatures of galaxy clusters from hydrodynamical<i>N</i>-body simulations to<i>Chandra</i>and<i>XMM-Newton</i>observations
Theoretical studies of the physical processes guiding the formation and evolution of galaxies and galaxy clusters in the X-ray are mainly based on the results of numerical hydrodynamical N-body simulations, which in turn are often directly compared to X-ray observations. Although trivial in principle, these comparisons are not always simple. …