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Simulating gamma-ray emission in star-forming galaxies

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Star-forming galaxies emit GeV and TeV gamma-rays that are thought to originate from hadronic interactions of cosmic-ray (CR) nuclei with the interstellar medium. To understand the emission, we have used the moving-mesh code Arepo to perform magnetohydrodynamical galaxy formation simulations with se...

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Bibliographic Details
Main Authors: Pfrommer, Christoph (Author) , Springel, Volker (Author)
Format: Article (Journal)
Language:English
Published: 2017 September 25
In: The astrophysical journal. Part 2, Letters
Year: 2017, Volume: 847, Issue: 2
ISSN:2041-8213
DOI:10.3847/2041-8213/aa8bb1
Online Access:Verlag, Volltext: http://dx.doi.org/10.3847/2041-8213/aa8bb1
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Author Notes:Christoph Pfrommer, Rüdiger Pakmor, Christine M. Simpson, and Volker Springel
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Simulating gamma-ray emission in star-forming galaxies by Pfrommer, Christoph (Author) , Springel, Volker (Author) ,


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