no code implementations • 10 Feb 2006 • F. Vazza, G. Tormen, R. Cassano, G. Brunetti, K. Dolag
We present a study of the turbulent velocity fields in the Intra Cluster Medium of a sample of 21 galaxy clusters simulated by the SPH--code Gadget2, using a new numerical scheme where the artificial viscosity is suppressed outside shocks.
