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Simulating galaxy formation with black hole driven thermal and kinetic feedback

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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 baryons has however p...

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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 P. (Author) , Torrey, Paul (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: February 2017
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1607.03486
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Author Notes:Rainer Weinberger, Volker Springel, Lars Hernquist, Annalisa Pillepich, Federico Marinacci, Rüdiger Pakmor, Dylan Nelson, Shy Genel, Mark Vogelsberger, Jill Naiman, Paul Torrey
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Simulating galaxy formation with black hole driven thermal and kinetic feedback by 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 P. (Author) , Torrey, Paul (Author) ,


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