Cluster Heating by AGN Outflows

Mathematics – Logic

Scientific paper

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Scientific paper

We present hydrodynamical simulations of the interaction between AGN jets and gas in a galaxy cluster. Simulations cover a range of AGN luminosities from 1044 to 1047 ergs/s. Morphological comparisons with X-ray and radio observations allow us to assess the importance of large scales motions within the cluster on the evolution of bubbles created by the AGN. We find that multipe bubbles can be created by a single episode of AGN activity. We also present a quantitative analysis of energy deposition by the AGN into the cluster gas.

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