Project Details
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Interactions between Active Galactic Nuclei and the Intracluster Medium

Subject Area Astrophysics and Astronomy
Term from 2005 to 2012
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 5447455
 
Final Report Year 2012

Final Report Abstract

The interaction between active galactic nuclei (AGN) and the intracluster medium (ICM) is essential for feedback, which is believed to be the crucial ingredient for the baryonic part of galaxy formation. In our project we made substantial progress in understanding the physics of AGN feedback: We characterised the AGN-ICM interactions in M87, Hydra A and M84 by a concerted approach of observations and hydrodynamic simulations, we found that turbulence is responsible for shaping the evolution of the AGN inflated bubbles and we are incorporating AGN feedback in cosmological simulations. AGN activity is not the only dynamical process in galaxy clusters that affects the state of the ICM, but galaxy clusters suffer major and minor mergers. Minor mergers lead to characteristic cold fronts wrapped around cluster cores. We have combined hydrodynamical simulations and observations to disentangle the merger history of Virgo and A496 from the properties of their cold fronts. Furthermore, the cluster galaxies continuously move through the ICM, and we have simulated ram pressure stripping of spiral galaxies and investigated the fate of their remaining gas disks and the properties of their wakes.

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