Low- and High-velocity O vi in Milky Way-like Galaxies: The Role of Stellar Feedback
Milky Way-type galaxies are surrounded by a warm-hot gaseous halo containing a considerable amount of baryons and metals. The kinematics and spatial distribution of highly ionized ion species such as O vi can be significantly affected by supernova (SN) explosions and early (pre-SN) stellar feedback...
| Autors principals: | , , , , , , , , , |
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| Format: | Article |
| Idioma: | English |
| Publicat: |
IOP Publishing
2024-01-01
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| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ad10a4 |