Modeling Agn Feedback In Cosmological Simulations

Details Modeling Agn Feedback In Cosmological Simulations Modeling Agn Feedback In Cosmological Simulations

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21840819a&link_type=abstract

American Astronomical Society, AAS Meeting #218, #408.19; Bulletin of the American Astronomical Society, Vol. 43, 2011

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We present results for the effects of thermal energy feedback from active galactic nuclei (AGN) in a Virgo size cluster using a series of cosmological hydrodynamic simulations. We examine the AGN's effect on early rapid black hole growth and its sensitivity to feedback model parameters. With AGN feedback, black hole accretion can reach a so-called 'self-regulating' phase. We find that this self-regulated behavior has important consequences in the role that ensuing mergers have on cooling flows towards the cluster center (r<20kpc).

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