AGN in Clusters of Galaxies - Berkeley Cosmology Group

More documents

Recommendations

Info

Hydra A AGN Feedback Observed X-ray Radio Cavities in the hot intracluster gas formed by radio jets McNamara et al. (2000)
Black Hole Evolution Rapid black hole growth produces an AGN An AGN requires: • triggering • fuel supply The cluster environment offers an opportunity to test this picture in the context of galaxy evolution Hopkins et al. (2005); Fan et al. (2001)
Page 1 and 2: AGN in Clusters of Galaxies Paul Ma
Page 3: Cluster Physics & the Cool Core Pro
Page 7 and 8: Galaxy Evolution in Clusters Do the
Page 9: Demographics Berlind et al. (2006)
Page 12 and 13: Mock Catalogs Create a mock catalog
Page 14 and 15: Radio Power at 1.4 GHz [w/Hz/sr] Lu
Page 16 and 17: Fraction of Sources < Projected Jet
Page 18: Distribution of AGN within Clusters
Page 21 and 22: Spectroscopic Confirmation Identifi
Page 23 and 24: AGN Identification LMXBs Hot Gas Jo
Page 25 and 26: Centrally Concentrated AGN Luminous
Page 27 and 28: Centrally Concentrated AGN Implicat
Page 29 and 30: AGN Fraction vs. Environment >95% p
Page 31 and 32: Field AGN Downsizing Silverman et a
Page 33 and 34: AGN in z>0.5 clusters
Page 35 and 36: Comparison to Field AGN More pronou
Page 37: Summary The FRII lifetime is ~10 7

AGN in Clusters of Galaxies - Berkeley Cosmology Group

Create successful ePaper yourself

Delete template?

Save as template?