High-velocity Molecular Clouds in M83

High-velocity clouds (HVCs), which are gas clouds moving at high velocity relative to the galactic disk, may play a critical role in galaxy evolution, potentially supplying gas to the disk and triggering star formation. In this study, we focus on the nearby face-on barred spiral galaxy M83, where hi...

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Bibliografiska uppgifter
Huvudupphovsmän: Maki Nagata, Fumi Egusa, Fumiya Maeda, Kazuki Tokuda, Kotaro Kohno, Kana Morokuma-Matsui, Jin Koda
Materialtyp: Artikel
Språk:engelska
Publicerad: IOP Publishing 2025-01-01
Serie:The Astrophysical Journal
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Länkar:https://doi.org/10.3847/1538-4357/addab7
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