The JWST-NIRCam View of Sagittarius C. II. Evidence for Magnetically Dominated H ii Regions in the Central Molecular Zone

We present JWST-NIRCam narrowband, 4.05 μ m Br α images of the Sgr C H ii region, located in the central molecular zone (CMZ) of the Galaxy. Unlike any H ii region in the solar vicinity, the Sgr C plasma is dominated by filamentary structure in both Br α and the radio continuum. Some bright filament...

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Autors principals:	John Bally, Samuel Crowe, Rubén Fedriani, Adam Ginsburg, Rainer Schödel, Morten Andersen, Jonathan C. Tan, Zhi-Yun Li, Francisco Nogueras-Lara, Yu Cheng, Chi-Yan Law, Q. Daniel Wang, Yichen Zhang, Suinan Zhang
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2025-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Emission nebulae
Accés en línia:	https://doi.org/10.3847/1538-4357/ad9d0b
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