Oral Presentation

Galaxy Clusters in the Magneticum Simulations

Author(s):

Presenter: Klaus Dolag (Ludwig-Maximilians University Munich)

I will present results from (GPc)^3 size, cosmological, hydro-dynamical simulations which follow the formation of cosmological structures
in so far unaccomplished detail, taking into account enough physical processes
to allow a self consistent comparison of galaxies, AGN and galaxy clusters to observations at multiple wavelength and throughout the entire epoch of structure formation (Magneticum, www.magneticum.org). Especially emphasis will be placed on galaxy clusters, where i will present results connecting evolution of satellite galaxies, the shape of the underlying dark matter halo, the ICM and the stellar component and how they are related to the formation history of the halos.