LoCuSS: A Dynamical Analysis Of X-ray AGN In Massive Clusters

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We present an analysis of the distribution of 48 X-ray AGN in 26 massive clusters at 0.15We show that the X-ray AGN found in massive clusters are an infalling population yet to encounter the dense ICM, and whose nuclear activity is very effectively shut down upon accretion into the cluster. These results are consistent with the view that for galaxy to host an X-ray AGN they should be the central galaxy within their dark matter halo, and have a ready supply of cold gas.

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