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Impact of AGNs on the Surrounding Medium
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The time- and ensemble-averaged mechanical energy outputs of radio galaxies may be large enough to offset much of the cooling inferred from X-ray observations of galaxy clusters. But does this heating actually counterbalance the cooling, diminishing cooling flows or quenching them altogether? I will argue that energy injection by radio galaxies may be important even in clusters where no active source is present, due to the likely intermittency of the jets. If the energy injected by radio galaxies percolates through the intracluster medium without excessive mixing, it could stabilize the atomic cooling responsible for X-ray emission.
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Cited by 2 Pith papers
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Decoding AGN Feedback with X-arithmetic: From Morphology to Physical Mechanisms
Applying X-arithmetic to 15 deeply observed Chandra halos, the authors classify AGN feedback structures and report multiple shocks in groups versus mainly isobaric structures around cavities in massive clusters.
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Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era
Perspective on using SKA-Low and SKA-Mid radio continuum to extend ram pressure stripping studies to southern clusters and z~0.5.
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