Taming the Tarantula: How Stellar Wind Feedback Shapes Gas and Dust in 30 Doradus

Observations of massive star-forming regions show that classical stellar wind models overpredict the luminosity of the X-ray-emitting gas, indicating a significant fraction of wind energy is lost. In this paper, we present a multiwavelength analysis of the giant H ii region 30 Doradus and its centra...

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Egile Nagusiak:	Jennifer A. Rodriguez, Laura A. Lopez, Lachlan Lancaster, Anna L. Rosen, Omnarayani Nayak, Sebastian Lopez, Tyler Holland-Ashford, Trinity L. Webb
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2026-01-01
Saila:	The Astrophysical Journal
Gaiak:	Interstellar medium Stellar wind bubbles H II regions Star formation
Sarrera elektronikoa:	https://doi.org/10.3847/1538-4357/ae3c7a
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