MagMaR III—Resisting the Pressure, Is the Magnetic Field Overwhelmed in NGC6334I?

We report on Atacama Large Millimeter/submillimeter Array observations of polarized dust emission at 1.2 mm from NGC6334I, a source known for its significant flux outbursts. Between five months, our data show no substantial change in total intensity and a modest 8% variation in linear polarization,...

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Dades bibliogràfiques

Autors principals:	Paulo C. Cortés, Josep M. Girart, Patricio Sanhueza, Junhao Liu, Sergio Martín, Ian W. Stephens, Henrik Beuther, Patrick M. Koch, M. Fernández-López, Álvaro Sánchez-Monge, Jia-Wei Wang, Kaho Morii, Shanghuo Li, Piyali Saha, Qizhou Zhang, David Rebolledo, Luis A. Zapata, Ji-hyun Kang, Wenyu Jiao, Jongsoo Kim, Yu Cheng, Jihye Hwang, Eun Jung Chung, Spandan Choudhury, A-Ran Lyo, Fernando Olguin
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2024-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Interstellar magnetic fields Star Formation Molecular Gas
Accés en línia:	https://doi.org/10.3847/1538-4357/ad59a7
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