Increasing Mass-to-flux Ratio from the Dense Core to the Protostellar Envelope around the Class 0 Protostar HH 211

Increasing Mass-to-flux Ratio from the Dense Core to the Protostellar Envelope around the Class 0 Protostar HH 211

To study the transportation of magnetic flux from large to small scales in protostellar sources, we analyzed the Nobeyama 45 m N _2 H ^+ (1–0), JCMT 850 μ m polarization, and Atacama Large Millimeter/submillimeter Array (ALMA) C ^18 O (2–1) and 1.3 and 0.8 mm (polarized) continuum data of the Class...

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Bibliographic Details
Main Authors: Hsi-Wei Yen, Patrick M. Koch, Chin-Fei Lee, Naomi Hirano, Nagayoshi Ohashi, Jinshi Sai (Insa Choi), Shigehisa Takakuwa, Ya-Wen Tang, Ken’ichi Tatematsu, Bo Zhao
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Star formation
Interstellar magnetic fields
Star forming regions
Protostars
Circumstellar disks
Online Access:https://doi.org/10.3847/1538-4357/aca47f

Internet

https://doi.org/10.3847/1538-4357/aca47f

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