Abstract

Contributed Talk - Splinter eROSITA

Galaxy Clusters from the Magneticum Simulations

K. Dolag1
1University Observatory Munich, Scheinerstrasse 1, 81679 Muenchen

Recent, cosmological hydrodynamical simulations can cover very large dynamical ranges in the resolved structures, while following a large variety of physical processes (e.g. star-formation, chemical enrichment, AGN feedback) which are important for the formation of galaxies and galaxy clusters. I will present the results from the "Magneticum" set of cosmological simulations with special emphasis on galaxy clusters. I will present results connecting the shape of the underlying dark matter halo, the ICM and the stellar component to the formation history of the halos.