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In large scale structure formation, massive systems assemble through thehierarchical merging of less massive ones. Galaxy clusters, being the mostmassive and thus the most recent collapsed structures, still grow by accretingsmaller clusters and groups. In order to investigate the dynamical evolution ofthe intracluster medium, we perform a set of adiabatic hydrodynamicalsimulations of binary cluster mergers.

Simulations of galaxy cluster mergers: the dynamics of Abell 3376