Magnetic Fields in the Central Molecular Zone Influenced by Feedback and Weakly Correlated with Star Formation

Magnetic Fields in the Central Molecular Zone Influenced by Feedback and Weakly Correlated with Star Formation

Magnetic fields of molecular clouds in the central molecular zone (CMZ) have been relatively under-observed at sub-parsec resolution. Here, we report JCMT/POL2 observations of polarized dust emission in the CMZ, which reveal magnetic field structures in dense gas at ∼0.5 pc resolution. The 11 molecu...

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Podrobná bibliografie
Hlavní autoři: Xing Lu, Junhao Liu, Thushara Pillai, Qizhou Zhang, Tie Liu, Qilao Gu, Tetsuo Hasegawa, Pak Shing Li, Xindi Tang, H Perry Hatchfield, Namitha Issac, Xunchuan Liu, Qiuyi Luo, Xiaofeng Mai, Zhiqiang Shen
Médium: Článek
Jazyk:English
Vydáno: IOP Publishing 2024-01-01
Edice:The Astrophysical Journal
Témata:
Interstellar magnetic fields
Molecular clouds
Galactic center
Star formation
On-line přístup:https://doi.org/10.3847/1538-4357/ad1395

Internet

https://doi.org/10.3847/1538-4357/ad1395

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