Low- and High-velocity O vi in Milky Way-like Galaxies: The Role of Stellar Feedback

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...

Deskribapen osoa

Xehetasun bibliografikoak
Egile Nagusiak: Zhijie Zhang, Xiaoxia Zhang, Hui Li, Taotao Fang, Qingzheng Yu, Yang Luo, Federico Marinacci, Laura V. Sales, Paul Torrey, Mark Vogelsberger
Formatua: Artikulua
Hizkuntza:English
Argitaratua: IOP Publishing 2024-01-01
Saila:The Astrophysical Journal
Gaiak:
High-velocity clouds
Interstellar medium
Warm ionized medium
Circumgalactic medium
Ultraviolet spectroscopy
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ad10a4

Internet

https://doi.org/10.3847/1538-4357/ad10a4

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