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FältnamnIndikatorerMetadata
00011199naa a2201525 4500
001oai:research.chalmers.se:7b117303-637e-4f03-8e7a-d7353c2fb036
003SwePub
008230105s2022 | |||||||||||000 ||eng|
024a https://doi.org/10.3847/1538-4357/ac99e02 DOI
024a https://research.chalmers.se/publication/5339952 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Hwang, Jihyeu Korea Astronomy and Space Science Institute,University of Science and Technology (UST)4 aut
2451 0a The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2
264 c 2022-12-12
264 1b American Astronomical Society,c 2022
338 a electronic2 rdacarrier
520 a We present and analyze observations of polarized dust emission at 850 μm toward the central 1 × 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 C18O (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 Alfvén 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.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Geovetenskap och miljövetenskapx Geofysik0 (SwePub)105052 hsv//swe
650 7a NATURAL SCIENCESx Earth and Related Environmental Sciencesx Geophysics0 (SwePub)105052 hsv//eng
650 7a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng
700a Kim, Jongsoou Korea Astronomy and Space Science Institute,University of Science and Technology (UST)4 aut
700a Pattle, Kateu University College London (UCL)4 aut
700a Lee, Chang Wonu University of Science and Technology (UST),Korea Astronomy and Space Science Institute4 aut
700a Koch, Patrick M.u Academia Sinica Taiwan4 aut
700a Johnstone, D.u University of Victoria,National Research Council Canada4 aut
700a Tomisaka, Kohjiu National Astronomical Observatory of Japan,The Graduate University for Advanced Studies (SOKENDAI)4 aut
700a Whitworth, Anthonyu Cardiff University4 aut
700a Furuya, Ray S.u Tokushima University4 aut
700a Kang, Ji-hyunu Korea Astronomy and Space Science Institute4 aut
700a Lyo, A.u Korea Astronomy and Space Science Institute4 aut
700a Chung, Eun Jungu Chungnam National University4 aut
700a Arzoumanian, Dorisu National Astronomical Observatory of Japan4 aut
700a Park, Geumsooku Korea Astronomy and Space Science Institute4 aut
700a Kwon, Woojinu Seoul National University4 aut
700a Kim, Shinyoungu Korea Astronomy and Space Science Institute4 aut
700a Tamura, Motohideu University of Tokyo, Japan,National Astronomical Observatory of Japan,National Institutes of Natural Sciences (NINS)4 aut
700a Kwon, Jungmiu University of Tokyo, Japan4 aut
700a Soam, Archanau Indian Institute of Astrophysics4 aut
700a Han, Ilseungu University of Science and Technology (UST),Korea Astronomy and Space Science Institute4 aut
700a Hoang, Thiemu Korea Astronomy and Space Science Institute,University of Science and Technology (UST)4 aut
700a Kim, Kyoung Heeu Korea Astronomy and Space Science Institute4 aut
700a Onaka, Takashiu University of Tokyo, Japan4 aut
700a Eswaraiah, Chakali4 aut
700a Ward-Thompson, D.u University of Central Lancashire4 aut
700a Liu, Hong-Liu Yunnan University4 aut
700a Tang, X. D.4 aut
700a Chen, Wen Pingu National Central University4 aut
700a Matsumura, Masafumiu Kagawa University4 aut
700a Hoang, Thuong Ducu University of Tokyo, Japan,Vietnam Academy of Science and Technology4 aut
700a Chen, Zhiweiu Chinese Academy of Sciences4 aut
700a Le Gouellec, Valentin J. M.u Université Paris-Saclay,University Paris-Saclay,Universities Space Research Association4 aut
700a Kirchschlager, F.u University College London (UCL)4 aut
700a Poidevin, Frédéricku Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna4 aut
700a Bastien, Pierreu Université de Montréal4 aut
700a Qiu, Kepingu Nanjing University4 aut
700a Hasegawa, Tetsuou National Astronomical Observatory of Japan4 aut
700a Lai, Shih-Pingu National Tsing Hua University,Academia Sinica Taiwan4 aut
700a Byun, Do Youngu Korea Astronomy and Space Science Institute,University of Science and Technology (UST)4 aut
700a Cho, Jungyeonu Chungnam National University4 aut
700a Choi, Minhou Korea Astronomy and Space Science Institute4 aut
700a Choi, Youngwoou Seoul National University4 aut
700a Choi, Yunheeu Korea Astronomy and Space Science Institute4 aut
700a Jeong, Il-Gyou Kyungpook National University,Korea Astronomy and Space Science Institute4 aut
700a Kang, Mijuu Korea Astronomy and Space Science Institute4 aut
700a Kim, Hyosungu Seoul National University4 aut
700a Kim, Kee-Taeu University of Science and Technology (UST),Korea Astronomy and Space Science Institute4 aut
700a Lee, Jeong Eunu Seoul National University4 aut
700a Lee, Sang Sungu Korea Astronomy and Space Science Institute,University of Science and Technology (UST)4 aut
700a Lee, Yong-Heeu East Asian Observatory,Kyung Hee University4 aut
700a Lee, Hyeseungu Chungnam National University4 aut
700a Kim, Mi-Ryangu Seoul National University4 aut
700a Yoo, Hyunjuu Chungnam National University4 aut
700a Yun, Hyeong-Siku Korea Astronomy and Space Science Institute4 aut
700a Chen, Michael Chun-Yuanu University of Victoria4 aut
700a Di Francesco, J.u University of Victoria,National Research Council Canada4 aut
700a Fiege, J.u University of Manitoba4 aut
700a Fissel, Laura M.u Queen's University4 aut
700a Franzmann, Ericau University of Manitoba4 aut
700a Lacaille, Kevinu McMaster University,Dalhousie University4 aut
700a Matthews, B. C.u National Research Council Canada,University of Victoria4 aut
700a Sadavoy, S. I.u Queen's University4 aut
700a Moriarty-Schieven, Gerald H.u National Research Council Canada4 aut
700a Tahani, M.u National Research Council Canada,Stanford University4 aut
700a Ching, Tao-Chung4 aut
700a Dai, Y. Sophiau Chinese Academy of Sciences4 aut
700a Duan, Yanu Chinese Academy of Sciences4 aut
700a Gu, Qilaou Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences4 aut
700a Law, Chi Yan,d 1990u Chinese University of Hong Kong,Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)ychi
700a Li, Dalei4 aut
700a Li, D.4 aut
700a Li, Guangxingu Yunnan University4 aut
700a Li, Hua-Baiu Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences4 aut
700a Liu, Tieu Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences4 aut
700a Lu, X.u Shanghai Astronomical Observatory. Chinese Academy of Sciences,Shanghai Astronomical Observatory Chinese Academy of Sciences4 aut
700a Qian, Leiu Chinese Academy of Sciences4 aut
700a Wang, Hongchiu Chinese Academy of Sciences4 aut
700a Wu, Jintaiu Nanjing University4 aut
700a Xie, Jinjinu Chinese Academy of Sciences4 aut
700a Yuan, Jinghuau Chinese Academy of Sciences4 aut
700a Zhang, Chuan-Pengu Chinese Academy of Sciences4 aut
700a Zhang, Guoyinu Chinese Academy of Sciences4 aut
700a Zhang, Yapengu Beijing Normal University4 aut
700a Zhou, Jianjun4 aut
700a Zhu, Leiu Chinese Academy of Sciences4 aut
700a Berry, Davidu East Asian Observatory4 aut
700a Friberg, P.u East Asian Observatory4 aut
700a Graves, Sarah F.u East Asian Observatory4 aut
700a Liu, Junhaou East Asian Observatory4 aut
700a Mairs, Steveu East Asian Observatory4 aut
700a Parsons, Harrietu East Asian Observatory4 aut
700a Rawlings, M.G.u East Asian Observatory,Gemini Observatory North4 aut
700a Doi, Yasuou University of Tokyo, Japan4 aut
700a Hayashi, Saekou National Astronomical Observatory of Japan4 aut
700a Hull, Charles L. H.u National Astronomical Observatory of Japan,Atacama Large Millimeter-submillimeter Array (ALMA)4 aut
700a Inoue, Tsuyoshi4 aut
700a Inutsuka, Shu-Ichirou Nagoya University4 aut
700a Iwasaki, Kazunariu Doshisha University4 aut
700a Kataoka, Akimasau National Astronomical Observatory of Japan4 aut
710a Korea Astronomy and Space Science Instituteb University of Science and Technology (UST)4 org
773t Astrophysical Journald : American Astronomical Societyg 941:1q 941:1x 1538-4357x 0004-637X
856u https://research.chalmers.se/publication/533995/file/533995_Fulltext.pdfx primaryx freey FULLTEXT
8564 8u https://doi.org/10.3847/1538-4357/ac99e0
8564 8u https://research.chalmers.se/publication/533995

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