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The role of cosmic ray pressure in accelerating galactic outflows

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We study the formation of galactic outflows from supernova explosions (SNe) with the moving-mesh code AREPO in a stratified column of gas with a surface density similar to the Milky Way disk at the solar circle. We compare different simulation models for SNe placement and energy feedback, including...

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Main Authors: Simpson, Christine M. (Author) , Pakmor, Rüdiger (Author) , Pfrommer, Christoph (Author) , Springel, Volker (Author) , Glover, Simon (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: August 17, 2016
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1606.02324
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Author Notes:Christine M. Simpson, Rüdiger Pakmor, Federico Marinacci, Christoph Pfrommer, Volker Springel, Simon C.O. Glover, Paul C. Clark and Rowan J. Smith
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The role of cosmic-ray pressure in accelerating galactic outflows by Simpson, Christine M. (Author) , Pakmor, Rüdiger (Author) , Pfrommer, Christoph (Author) , Springel, Volker (Author) , Glover, Simon (Author) ,


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