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How does environment affect the morphology of radio AGN?
Melissa Elizabeth Morris, Eric Wilcots, Eric Hooper +1
Galaxies hosting Active Galactic Nuclei (AGN) with bent radio jets are used as tracers of dense environments, such as galaxy groups and clusters. The assumption behind using these…
Jets, Bubbles, and Heat Pumps in Galaxy Clusters
Yi-Hao Chen, Sebastian Heinz, Torsten A. Enßlin
Feedback from AGN jets has been proposed to counteract the catastrophic cooling in many galaxy clusters. However, it is still unclear which physical processes are acting to couple…
Massive Compact Galaxies with High-Velocity Outflows: Morphological Analysis and Constraints on AGN Activity
P. H. Sell, C. A. Tremonti, R. C. Hickox +9
We investigate the process of rapid star formation quenching in a sample of 12 massive galaxies at intermediate redshift (z~0.6) that host high-velocity ionized gas outflows (v>100…
Evolution of X-ray cavities
Marcus Brüggen, Evan Scannapieco, Sebastian Heinz
A wide range of recent observations have shown that AGN-driven cavities may provide the energy source that balances the cooling observed in the centres of cool-core galaxy clusters…