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....

Bibliografski detalji
Glavni autori:	Kannan, Rahul, Vogelsberger, Mark, Pfrommer, Christoph, Weinberger, Rainer, Springel, Volker, Hernquist, Lars, Puchwein, Ewald, Pakmor, Rüdiger
Daljnji autori:	Massachusetts Institute of Technology. Department of Physics
Format:	Članak
Jezik:	en_US
Izdano:	IOP Publishing 2017
Online pristup:	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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