Simulating galaxy formation with black hole driven thermal and kinetic feedback

Simulating galaxy formation with black hole driven thermal and kinetic feedback

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© 2016 The Authors. The inefficiency of star formation in massive elliptical galaxies is widely believed to be caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas. Achieving a sufficiently rapid reddening of moderately massive galaxies without expelling too many b...

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Main Authors: Weinberger, Rainer (Author), Springel, Volker (Author), Hernquist, Lars (Author), Pillepich, Annalisa (Author), Marinacci, Federico (Author), Pakmor, Rüdiger (Author), Nelson, Dylan (Author), Genel, Shy (Author), Vogelsberger, Mark (Author), Naiman, Jill (Author), Torrey, Paul A. (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: Oxford University Press (OUP), 2022-07-22T14:42:54Z.
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