Gone With The Wind: Interactive Feedback In Galaxy Clusters

Details Gone With The Wind: Interactive Feedback In Galaxy Clusters Gone With The Wind: Interactive Feedback In Galaxy Clusters

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21112501h&link_type=abstract

American Astronomical Society, AAS Meeting #211, #125.01; Bulletin of the American Astronomical Society, Vol. 39, p.955

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The interaction of AGN jets with the intra-cluster medium is believed to be the primary feedback mechanism between growing supermassive black holes and their environment. It is now possible to simulate this interaction in realistic, cosmologically evolved cluster atmospheres, and, at the same time, with realistic, collimated jets. I will discuss the latest results from our campaign to model feedback in galaxy clusters, which now covers more than 2 orders of magnitude in jet power. I will further discuss recent results on the stability and dynamics of radio bubbles once the jets have turned off, a topic of great importance for the interpretation of X-ray observations of clusters.

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