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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 (SN) explosions 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 SN placement and energy feedback, including co...

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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)
Language:English
Published: 2016 August 16
In: The astrophysical journal. Part 2, Letters
Year: 2016, Volume: 827, Issue: 2
ISSN:2041-8213
DOI:10.3847/2041-8205/827/2/L29
Online Access:Verlag, Volltext: http://dx.doi.org/10.3847/2041-8205/827/2/L29
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Author Notes:Christine M. Simpson, Rüdiger f f per , 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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