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B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main | |
Kwon, Woojin1,2; Pattle, Kate3,4; Sadavoy, Sarah5; Hull, Charles L. H.6,7; Johnstone, Doug8,9; Ward-Thompson, Derek10; Di Francesco, James8,9; Koch, Patrick M.11; Furuya, Ray12,13; Doi, Yasuo14; Le Gouellec, Valentin J. M.15,16; Hwang, Jihye17,18; Lyo, A-Ran17; Soam, Archana15,19; Tang, Xindi20![]() ![]() ![]() ![]() | |
2022-02-01 | |
Source Publication | ASTROPHYSICAL JOURNAL
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ISSN | 0004-637X |
Volume | 926Issue:2Pages:163 |
Contribution Rank | 20 |
Abstract | We present 850 mu m polarimetric observations toward the Serpens Main molecular cloud obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope as part of the B-fields In STar-forming Region Observations survey. These observations probe the magnetic field morphology of the Serpens Main molecular cloud on about 6000 au scales, which consists of cores and six filaments with different physical properties such as density and star formation activity. Using the histogram of relative orientation (HRO) technique, we find that magnetic fields are parallel to filaments in less-dense filamentary structures where NH2 < 0.93 x 10(22) cm(-2) (magnetic fields perpendicular to density gradients), while they are perpendicular to filaments (magnetic fields parallel to density gradients) in dense filamentary structures with star formation activity. Moreover, applying the HRO technique to denser core regions, we find that magnetic field orientations change to become perpendicular to density gradients again at NH2 approximate to 4.6 x 10(22) NH2 approximate to 16 x 10(22) cm(-2), magnetic fields change back to being parallel to density gradients once again, which can be understood to be due to magnetic fields being dragged in by infalling material. In addition, we estimate the magnetic field strengths of the filaments (B-POS = 60-300 mu G)) using the Davis-Chandrasekhar-Fermi method and discuss whether the filaments are gravitationally unstable based on magnetic field and turbulence energy densities. |
DOI | 10.3847/1538-4357/ac4bbe |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | IMAGING POLARIMETRY ; INTERSTELLAR CLOUDS ; SCUBA-2 ; POLARIZATION ; SPITZER ; LEGACY ; ORION ; 1ST ; STRENGTHS ; ALIGNMENT |
Funding Project | National Key R&D Program of China[2017YFA0402700] ; National Key R&D Program of China[2017YFA0402600] ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; New Faculty Startup Fund from Seoul National University ; National Research Foundation of Korea (NRF) - Korean government (MSIT)[NRF-2021R1F1A1061794] ; NRC Canada ; NSERC ; NAOJ Fellowship ; JSPS KAKENHI[18K13586] ; JSPS KAKENHI[20K14527] ; JSPS KAKENHI[18H05442] ; JSPS KAKENHI[15H02063] ; JSPS KAKENHI[22000005] ; National Natural Science Foundation of China (NSFC) grant[U1731237] ; Basic Science Research Program through the NRF - Ministry of Education, Science and Technology[NRF-2019R1A2C1010851] ; Science and Engineering Research Board (SERB), Department of Science and Technology (DST), Govt. of India[RJF/2020/000071] ; Ministry of Science and Technology of Taiwan[AS-IA-106-M03] ; Ministry of Science and Technology of Taiwan[106-2119-M-007-021-MY3] ; Ministry of Science and Technology of Taiwan[109-2112-M-007-010-MY3] ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education[NRF-2020R1A6A3A01100208] ; National Research Foundation of Korea (NRF) grant - Korean government (MSIT) through the Mid-career Research Program[2019R1A2C1087045] ; [M16AL004] ; [URF\R1\211322] ; [MOST 108-2112-M-001-004-MY2] |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000759830000001 |
Publisher | IOP Publishing Ltd |
Funding Organization | National Key R&D Program of China ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; New Faculty Startup Fund from Seoul National University ; National Research Foundation of Korea (NRF) - Korean government (MSIT) ; NRC Canada ; NSERC ; NAOJ Fellowship ; JSPS KAKENHI ; National Natural Science Foundation of China (NSFC) grant ; Basic Science Research Program through the NRF - Ministry of Education, Science and Technology ; Science and Engineering Research Board (SERB), Department of Science and Technology (DST), Govt. of India ; Ministry of Science and Technology of Taiwan ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education ; National Research Foundation of Korea (NRF) grant - Korean government (MSIT) through the Mid-career Research Program |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/4508 |
Collection | 射电天文研究室_恒星形成与演化研究团组 |
Corresponding Author | Kwon, Woojin |
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Recommended Citation GB/T 7714 | Kwon, Woojin,Pattle, Kate,Sadavoy, Sarah,et al. B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main[J]. ASTROPHYSICAL JOURNAL,2022,926(2):163. |
APA | Kwon, Woojin.,Pattle, Kate.,Sadavoy, Sarah.,Hull, Charles L. H..,Johnstone, Doug.,...&van Loo, Sven.(2022).B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main.ASTROPHYSICAL JOURNAL,926(2),163. |
MLA | Kwon, Woojin,et al."B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main".ASTROPHYSICAL JOURNAL 926.2(2022):163. |
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