Stellar winds and photoionization in a spiral arm

The role of different stellar feedback mechanisms in giant molecular clouds is not well understood. This is especially true for regions with many interacting clouds as would be found in a galactic spiral arm. In this paper, building on previous work by Bending et al., we extract a \(500\times500\tim...

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Veröffentlicht in:	arXiv.org 2022-01
Hauptverfasser:	Ali, Ahmad A, Bending, Thomas J R, Dobbs, Clare L
Format:	Artikel
Sprache:	eng
Schlagworte:	Deposition Feedback Massive stars Molecular clouds Photoionization Physics - Astrophysics of Galaxies Smooth particle hydrodynamics Star & galaxy formation Star formation rate Stellar winds
Online-Zugang:	Volltext
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