Cosmic rays across the star-forming galaxy sequence – II. Stability limits and the onset of cosmic ray-driven outflows
ABSTRACT Cosmic rays (CRs) are a plausible mechanism for launching winds of cool material from the discs of star-forming galaxies. However, there is no consensus on what types of galaxies likely host CR-driven winds, or what role these winds might play in regulating galaxies’ star formation rates. U...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2021-05, Vol.503 (2), p.2651-2664 |
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Sprache: | eng |
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