Gas density (left), X-ray emission weighted temperature (center), and entropy radial profiles (left) obtained at several epochs during the cluster evolution in run K1. The comparison with the other runs is shown in Fig. A.1. The additional gray lines show the distribution of corresponding profiles obtained from the ACCEPT sample by Cavagnolo et al. (2009) for clusters with a central temperature in a range of 3 ≤ T ≤ 5 KeV and a central entropy less than 50 KeV/cm² meant to select cool core cluster with masses close to the simulated Perseus-like cluster.