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Chinese Academy of Sciences Institutional Repositories Grid
The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2

文献类型:期刊论文

作者Hwang, Jihye98,99; Kim, Jongsoo98,99; Pattle, Kate97; Lee, Chang Won98,99; Koch, Patrick M.96; Johnstone, Doug94,95; Tomisaka, Kohji91,92; Whitworth, Anthony90; Furuya, Ray S.89; Kang, Ji-hyun99
刊名Astrophysical Journal
出版日期2022-12-01
卷号941期号:1页码:1951
ISSN号0004-637X
关键词dense cores scuba-2 1st polarization gravity regions clouds pol-2 model Astronomy & Astrophysics
DOI10.3847/1538-4357/ac99e0
产权排序24
文献子类Article
英文摘要We present and analyze observations of polarized dust emission at 850 mu m toward the central 1 x 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obtained with SCUBA-2/POL-2 on the James Clerk Maxwell Telescope (JCMT) as part of the B-fields in Star-forming Region Observations survey. The orientations of the magnetic field follow the spiral structure of Mon R2, which are well described by an axisymmetric magnetic field model. We estimate the turbulent component of the magnetic field using the angle difference between our observations and the best-fit model of the underlying large-scale mean magnetic field. This estimate is used to calculate the magnetic field strength using the Davis-Chandrasekhar-Fermi method, for which we also obtain the distribution of volume density and velocity dispersion using a column density map derived from Herschel data and the (CO)-O-18 (J = 3 - 2) data taken with HARP on the JCMT, respectively. We make maps of magnetic field strengths and mass-to-flux ratios, finding that magnetic field strengths vary from 0.02 to 3.64 mG with a mean value of 1.0 +/- 0.06 mG, and the mean critical mass-to-flux ratio is 0.47 +/- 0.02. Additionally, the mean Alfven Mach number is 0.35 +/- 0.01. This suggests that, in Mon R2, the magnetic fields provide resistance against large-scale gravitational collapse, and the magnetic pressure exceeds the turbulent pressure. We also investigate the properties of each filament in Mon R2. Most of the filaments are aligned along the magnetic field direction and are magnetically subcritical.
语种英语
WOS记录号WOS:000927885400001
源URL[http://ir.xao.ac.cn/handle/45760611-7/5135]  
专题恒星形成与演化研究团组
作者单位1.Department of Physics and Astronomy, The University of Western Ontario, 1151 Richmond Street, London N6A 3K7, Canada;
2.Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
3.National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USA;
4.Jet Propulsion Laboratory, M/S 169-506, 4800 Oak Grove Drive, Pasadena, CA 91109, USA;
5.Laboratoire AIM CEA/DSM-CNRS-Université Paris Diderot, IRFU/Service d’Astrophysique, CEA Saclay, F-91191 Gif-sur-Yvette, France;
6.Graduate University of Science and Technology, Vietnam Academy of Science and Technology, 18 Hoang Quoc Viet, Cau Giay, Hanoi, Vietnam;
7.Vietnam National Space Center, Vietnam Academy of Science and Technology, 18 Hoang Quoc Viet, Hanoi, Vietnam;
8.OSL, Physics & Astronomy Dept., University College London, WC1E 6BT London, UK;
9.Kavli Institute for Cosmology, Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK;
10.Astrophysics Group, Cavendish Laboratory, J.J. Thomson Avenue, Cambridge CB3 0HE, UK;
推荐引用方式
GB/T 7714
Hwang, Jihye,Kim, Jongsoo,Pattle, Kate,et al. The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2[J]. Astrophysical Journal,2022,941(1):1951.
APA Hwang, Jihye.,Kim, Jongsoo.,Pattle, Kate.,Lee, Chang Won.,Koch, Patrick M..,...&Robitaille, Jean-Francois.(2022).The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2.Astrophysical Journal,941(1),1951.
MLA Hwang, Jihye,et al."The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2".Astrophysical Journal 941.1(2022):1951.

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