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most citedN-body simulations for coupled dark energy: halo mass function and density profiles

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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…