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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Bibliographic Details
Main Authors: Kannan, Rahul, Vogelsberger, Mark, Pfrommer, Christoph, Weinberger, Rainer, Springel, Volker, Hernquist, Lars, Puchwein, Ewald, Pakmor, Rüdiger
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2017
Online Access:http://hdl.handle.net/1721.1/109697
https://orcid.org/0000-0002-3074-2326
https://orcid.org/0000-0001-8593-7692

Internet

http://hdl.handle.net/1721.1/109697
https://orcid.org/0000-0002-3074-2326
https://orcid.org/0000-0001-8593-7692

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