Mass-loading and non-spherical divergence in hot galactic winds: implications for X-ray observations
ABSTRACT Cool clouds are expected to be destroyed and incorporated into hot supernova-driven galactic winds. The mass-loading of a wind by the cool medium modifies the bulk velocity, temperature, density, entropy, and abundance profiles of the hot phase relative to an unmass-loaded outflow. We provi...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2021-12, Vol.508 (4), p.5310-5325 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
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