From the Outskirts of Galaxies to Intra Cluster Light
Abstract
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.
- Publication:
-
The General Assembly of Galaxy Halos: Structure, Origin and Evolution
- Pub Date:
- August 2016
- DOI:
- 10.1017/S1743921315010467
- Bibcode:
- 2016IAUS..317..292D
- Keywords:
-
- hydrodynamics;
- numerical;
- galaxy: formation;
- clusters;
- dynamics