Abstract

Contributed Talk - Splinter eROSITA

Thursday, 21 September 2017, 18:00   (HS4)

Galaxy Clusters from the Magneticum Simulations

K. Dolag^1
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.