The JCMT BISTRO Survey: Unveiling the Magnetic Fields around Galactic Center

Abstract We acquired 450 and 850 μ m dust continuum polarization observations toward the inner region of the Central Molecular Zone (CMZ) as part of the B -Fields In Star-forming Region Observations survey using the POL-2 polarimeter on the James Clerk Maxwell Telescope. These observations encompassed three dense structures: the 20 km s −1 cloud (20MC), 50 km s −1 cloud (50MC), and circumnuclear disk (CND). Our aim is to investigate the magnetic field morphology and strength in the inner region of the CMZ using polarized dust continuum and the Davis–Chandrasekhar–Fermi method. The magnetic field morphology is highly ordered in all three dense regions. The plane-of-sky magnetic field strengths are ∼1 mG for the 20MC and the 50MC, and ∼2 mG for the CND. We compare the energy contributions of turbulence, gravity, and thermal motion with that of the magnetic field using the plasma β , mass-to-flux ratio, and Alfvén Mach number. The outcomes reveal the magnetic field stands out as the predominant factor within the inner region of the CMZ. The dominance of the magnetic field may explain the low star-forming rate in the CMZ. We further investigate the dust grain alignment efficiency by exploring the relationship between polarization fraction and total intensity. The results suggest that dust grains are well aligned with the magnetic fields.

Authors

Publication Details

Journal
The Astrophysical Journal
Published
2025-04-18
DOI
https://doi.org/10.3847/1538-4357/adbe34
Citations
3
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
3.46
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article

The JCMT BISTRO Survey: Unveiling the Magnetic Fields around Galactic Center

Tie Liu, Jihye Hwang, D. Ward–Thompson, G. A. Fuller et al.
3 citations
The Astrophysical Journal
Stellar, planetary, and galactic studies
3.46
article

The JCMT BISTRO Survey: Unveiling the Magnetic Fields around Galactic Center

Tie Liu, Jihye Hwang, D. Ward–Thompson, G. A. Fuller, S. Lai, Simon Coudé, Jungmi Kwon, Tetsuo Hasegawa, Lapo Fanciullo, Takashi Onaka, Ji‐hyun Kang, Thiem Hoang, Patrick M. Koch, Janik Karoly, David J. Eden, Yasuo Doi, Pierre Bastien, Chang Won Lee, David Berry, Xing Lu, Woojin Kwon, Guang-Xing Li, Kate Pattle, M. S. Akshaya, D. Arzoumanian, Keping Qiu, Sarah Sadavoy, Shu‐ichiro Inutsuka, James Di Francesco, Valentin J. M. Le Gouellec, Motohide Tamura, Qilao Gu, F. Poidevin, Ekta Sharma, Mehrnoosh Tahani, Hao-Yuan Duan, Le Ngoc Tram, Ray S. Furuya, Jia-Wei Wang, Junhao Liu, Sheng-Jun Lin, Meng-Zhe Yang, Bijas Najimudeen
article en
3 citations

Abstract

Abstract We acquired 450 and 850 μ m dust continuum polarization observations toward the inner region of the Central Molecular Zone (CMZ) as part of the B -Fields In Star-forming Region Observations survey using the POL-2 polarimeter on the James Clerk Maxwell Telescope. These observations encompassed three dense structures: the 20 km s −1 cloud (20MC), 50 km s −1 cloud (50MC), and circumnuclear disk (CND). Our aim is to investigate the magnetic field morphology and strength in the inner region of the CMZ using polarized dust continuum and the Davis–Chandrasekhar–Fermi method. The magnetic field morphology is highly ordered in all three dense regions. The plane-of-sky magnetic field strengths are ∼1 mG for the 20MC and the 50MC, and ∼2 mG for the CND. We compare the energy contributions of turbulence, gravity, and thermal motion with that of the magnetic field using the plasma β , mass-to-flux ratio, and Alfvén Mach number. The outcomes reveal the magnetic field stands out as the predominant factor within the inner region of the CMZ. The dominance of the magnetic field may explain the low star-forming rate in the CMZ. We further investigate the dust grain alignment efficiency by exploring the relationship between polarization fraction and total intensity. The results suggest that dust grains are well aligned with the magnetic fields.

The Astrophysical JournalVol. 983(2)
Openalex Percentile: Top 8%
Stellar, planetary, and galactic studies
3.46
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