The Effect of Radiative Cooling on Scaling Relations of X-ray Clusters

Abstract

We have performed cosmological simulations in a ΛCDM cosmology with and without radiative cooling, in order to study the effect of cooling on the cluster scaling relations. Our simulations consist of 4.1 million particles each of gas and dark matter within a box-size of 100 h−1 Mpc and the run with cooling is the largest of its kind to have been evolved to… (More)

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