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From the Outskirts of Galaxies to Intra Cluster Light

Published online by Cambridge University Press:  09 May 2016

Klaus Dolag ,
Rhea-Silvia Remus  and
Adelheid F. Teklu
Klaus Dolag
Affiliation:
Universitäts-Sternwarte München, Scheinerstrasse 1, München, Germany email: dolag@usm.uni-muenchen.de
Rhea-Silvia Remus
Affiliation:
Universitäts-Sternwarte München, Scheinerstrasse 1, München, Germany email: dolag@usm.uni-muenchen.de
Adelheid F. Teklu
Affiliation:
Universitäts-Sternwarte München, Scheinerstrasse 1, München, Germany email: dolag@usm.uni-muenchen.de
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Abstract

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We use the Magneticum Pathfinder (www.magneticum.org) hydro-dynamical cosmological simulation set to investigate the buildup of the stellar component within cosmological structures. These simulations result in the self-consistent formation of ICM, AGNs, and both spheroidal and disk galaxy populations, which properly reproduce the observed properties.

Keywords

hydrodynamicsnumericalgalaxy: formationclustersdynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Issue S317: The General Assembly of Galaxy Halos: Structure, Origin and Evolution , August 2015 , pp. 292 - 293
Copyright
Copyright © International Astronomical Union 2016 

References

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