BISTRO Survey: Gravity-dominated and Magnetically Regulated Star Formation in M17 SW

We present high-resolution magnetic field maps of the M17 SW molecular cloud using JCMT 850 μ m dust polarization at scale of 14″. The magnetic field exhibits a distinct arc-like structure that encircles three dense clumps (C1, C2, and C3). By combining polarization data with ammonia line observatio...

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Xehetasun bibliografikoak

Egile Nagusiak:	Mengke Zhao, Keping Qiu, Ji-hyun Kang, Xindi Tang, Anthony Whitworth, Derek Ward-Thompson, Takashi Onaka, Chang Won Lee, Tyler L. Bourke, Jihye Hwang, David Eden, Thiem Hoang, Motohide Tamura, Jungmi Kwon, Felix Priestley, Kee-Tae Kim, Doris Arzoumanian, James Di Francesco, Chakali Eswaraiah, Doug Johnstone, Bich Ngoc Nguyen, Zhiwei Chen, Sarah Sadavoy, Archana Soam, Ray S. Furuya, Shih-Ping Lai, Woojin Kwon, Pierre Bastien, Kate Pattle, David Berry
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2026-01-01
Saila:	The Astrophysical Journal
Gaiak:	Interstellar magnetic fields Star formation Interstellar clouds
Sarrera elektronikoa:	https://doi.org/10.3847/1538-4357/ae6ce5
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