Geometry, Dissipation, Cooling, and the Dynamical Evolution of Wind-blown Bubbles

Bubbles driven by energy and mass injection from small scales are ubiquitous in astrophysical fluid systems and essential to feedback across multiple scales. In particular, O stars in young clusters produce high-velocity winds that create hot bubbles in the surrounding gas. We demonstrate that the d...

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Détails bibliographiques

Auteurs principaux:	Lachlan Lancaster, Eve C. Ostriker, Chang-Goo Kim, Jeong-Gyu Kim, Greg L. Bryan
Format:	Artigo
Langue:	Inglês
Publié:	IOP Publishing 2024-01-01
Collection:	The Astrophysical Journal
Sujets:	Stellar winds Interstellar medium Star forming regions Stellar feedback Stellar wind bubbles Young star clusters
Accès en ligne:	https://doi.org/10.3847/1538-4357/ad47f6
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