Gas density (left panels), X-ray emission weighted temperature (center panels), and entropy radial profiles (left panels) obtained at several epochs during the cluster evolution in runs K1, K05, K05_np, K01, K01_np, and K1_np (from top to bottom). 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 50KeV/cm² meant to select cool core cluster with masses close to the Perseus-like cluster simulated.