Galactic winds driven by isotropic and anisotropic cosmic-ray diffusion in disk galaxies
The physics of cosmic rays (CRs) is a promising candidate for explaining the driving of galactic winds and outflows. Recent galaxy formation simulations have demonstrated the need for active CR transport either in the form of diffusion or streaming to successfully launch winds in galaxies. However,...
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| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2016 June 21
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| In: |
The astrophysical journal. Part 2, Letters
Year: 2016, Jahrgang: 824, Heft: 2 |
| ISSN: | 2041-8213 |
| DOI: | 10.3847/2041-8205/824/2/L30 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.3847/2041-8205/824/2/L30
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| Verfasserangaben: | R. Pakmor, C. Pfrommer, C.M. Simpson, and V. Springel |
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Galactic winds driven by isotropic and anisotropic cosmic ray diffusion in disk galaxies
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