2 papers
astro-ph2002
Iron abundances in hydrodynamical simulations of galaxy clusters
R. Valdarnini
Hydrodynamical SPH simulations of galaxy clusters are used to investigate the metal enrichment of the intracluster medium. The final metallicity abundances of the simulated cluster…
astro-ph2000
Morphological evolution of X-ray clusters using hydrodynamical simulations
R. Valdarnini, S. Ghizzardi, S. Bonometto
A large set of TREESPH simulations is used to test the global morphology of galaxy clusters and its evolution against X-ray data. A powerful method to investigate substructures in…