Increasing Black Hole Feedback-induced Quenching with Anisotropic Thermal Conduction

Increasing Black Hole Feedback-induced Quenching with Anisotropic Thermal Conduction

Feedback from central supermassive black holes is often invoked to explain the low star formation rates (SFRs) in the massive galaxies at the centers of galaxy clusters. However, the detailed physics of the coupling of the injected feedback energy with the intracluster medium (ICM) is still unclear....

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Main Authors: Kannan, Rahul (Contributor), Vogelsberger, Mark (Contributor), Pfrommer, Christoph (Author), Weinberger, Rainer (Author), Springel, Volker (Author), Hernquist, Lars (Author), Puchwein, Ewald (Author), Pakmor, Rüdiger (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-06-07T13:48:34Z.
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