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| A Tale of Three: Magnetic Fields along the Orion Integral-shaped Filament as Revealed by the JCMT BISTRO Survey | |
Wu, Jintai1,2; Qiu, Keping1,2; Poidevin, Frederick3,4; Bastien, Pierre5,6; Liu, Junhao7; Ching, Tao-Chung8; Bourke, Tyler L.9,10; Ward-Thompson, Derek11; Pattle, Kate12; Johnstone, Doug13,14; Koch, Patrick M.15; Arzoumanian, Doris16; Lee, Chang Won17,18; Fanciullo, Lapo19; Onaka, Takashi20; Hwang, Jihye17; Le Gouellec, Valentin J. M.21,22; Soam, Archana23; Tamura, Motohide20,24,25; Tahani, Mehrnoosh26; Eswaraiah, Chakali27; Li, Hua-Bai28; Berry, David29; Furuya, Ray S.30; Coude, Simon31,32; Kwon, Woojin33,34,35; Lin, Sheng-Jun15; Wang, Jia-Wei15; Hasegawa, Tetsuo24; Lai, Shih-Ping15,36,37; Byun, Do-Young17,18; Chen, Zhiwei38; Chen, Huei-Ru Vivien15,36,37; Chen, Wen Ping39; Chen, Mike14; Cho, Jungyeon40; Choi, Youngwoo41; Choi, Yunhee17; Choi, Minho17; Chrysostomou, Antonio9; Chung, Eun Jung17; Dai, Sophia42; Di Francesco, James13,14; Pham Ngoc Diep43; Doi, Yasuo44; Duan, Hao-Yuan45; Duan, Yan42; Eden, David46; Fiege, Jason47; Fissel, Laura M.48; Franzmann, Erica47; Friberg, Per29; Friesen, Rachel49; Fuller, Gary10; Gledhill, Tim50; Graves, Sarah29; Greaves, Jane51; Griffin, Matt51; Gu, Qilao52; Han, Ilseung17,18; Hayashi, Saeko53; Hoang, Thiem17,18; Houde, Martin54; Inoue, Tsuyoshi55; Inutsuka, Shu-ichiro56; Iwasaki, Kazunari57; Jeong, Il-Gyo17,58; Koenyves, Vera11; Kang, Ji-hyun17; Kang, Miju17; Karoly, Janik12; Kataoka, Akimasa59; Kawabata, Koji60,61,62; Kim, Shinyoung17; Kim, Mi-Ryang63; Kim, Kyoung Hee64; Kim, Kee-Tae17,18; Kim, Jongsoo17,18; Kim, Hyosung33; Kim, Gwanjeong65; Kirchschlager, Florian66; Kirk, Jason11; Kobayashi, Masato I. N.67; Kusune, Takayoshi68; Kwon, Jungmi20; Lacaille, Kevin69,70; Law, Chi-Yan28,71; Lee, Hyeseung72; Lee, Chin-Fei15; Lee, Sang-Sung17,18; Lee, Jeong-Eun73; Li, Dalei74 ; Li, Di75,76; Li, Guangxing77; Liu, Sheng-Yuan15; Liu, Tie78; Liu, Hong-Li79; Lu, Xing52; Lyo, A-Ran17; Mairs, Steve29; Matsumura, Masafumi80,81; Matthews, Brenda13,14; Moriarty-Schieven, Gerald13; Nagata, Tetsuya82; Nakamura, Fumitaka59,83; Nakanishi, Hiroyuki84; Nguyen Bich Ngoc43,85; Ohashi, Nagayoshi15; Park, Geumsook17; Parsons, Harriet29; Peretto, Nicolas51; Priestley, Felix51; Pyo, Tae-Soo83,86; Qian, Lei75; Rao, Ramprasad15; Rawlings, Jonathan12; Rawlings, Mark29,87; Retter, Brendan51; Richer, John88,89; Rigby, Andrew51; Sadavoy, Sarah48; Saito, Hiro90; Savini, Giorgio91; Seta, Masumichi92; Sharma, Ekta75; Shimajiri, Yoshito93; Shinnaga, Hiroko84; Tang, Ya-Wen15; Tang, Xindi94; Hoang Duc Thuong95; Tomisaka, Kohji59; Le Ngoc Tram96; Tsukamoto, Yusuke84; Viti, Serena97; Wang, Hongchi38; Whitworth, Anthony51; Xie, Jinjin42; Yang, Meng-Zhe36,37; Yen, Hsi-Wei15; Yoo, Hyunju40; Yuan, Jinghua42; Yun, Hyeong-Sik17; Zenko, Tetsuya82; Zhang, Guoyin75; Zhang, Chuan-Peng42,75; Zhang, Yapeng98; Zhou, Jianjun74; Zhu, Lei75; de Looze, Ilse66; Andre, Philippe99; Dowell, C. Darren100; Eyres, Stewart101; Falle, Sam102; Robitaille, Jean-Francois103; van Loo, Sven104
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| 2024-12-20 | |
| Source Publication | ASTROPHYSICAL JOURNAL LETTERS
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| ISSN | 2041-8205 |
| Volume | 977Issue:2Pages:14 |
| Abstract | As part of the B-fields In Star-forming Region Observations survey, we present James Clerk Maxwell Telescope (JCMT) 850 mu m polarimetric observations toward the Orion integral-shaped filament (ISF) that covers three portions known as OMC-1, OMC-2, and OMC-3. The magnetic field threading the ISF seen in the JCMT POL-2 map appears as a tale of three: pinched for OMC-1, twisted for OMC-2, and nearly uniform for OMC-3. A multiscale analysis shows that the magnetic field structure in OMC-3 is very consistent at all the scales, whereas the field structure in OMC-2 shows no correlation across different scales. In OMC-1, the field retains its mean orientation from large to small scales but shows some deviations at small scales. Histograms of relative orientations between the magnetic field and filaments reveal a bimodal distribution for OMC-1, a relatively random distribution for OMC-2, and a distribution with a predominant peak at 90 degrees for OMC-3. Furthermore, the magnetic fields in OMC-1 and OMC-3 both appear to be aligned perpendicular to the fibers, which are denser structures within the filament, but the field in OMC-2 is aligned along with the fibers. All these suggest that gravity, turbulence, and magnetic field are each playing a leading role in OMC-1, 2, and 3, respectively. While OMC-2 and 3 have almost the same gas mass, density, and nonthermal velocity dispersion, there are on average younger and fewer young stellar objects in OMC-3, providing evidence that a stronger magnetic field will induce slower and less efficient star formation in molecular clouds. |
| Corresponding Author | Qiu, Keping(kpqiu@nju.edu.cn) |
| DOI | 10.3847/2041-8213/ad93d2 |
| Indexed By | SCI ; SCI |
| Language | 英语 |
| WOS Keyword | FORMING MOLECULAR CLOUDS ; STAR-FORMATION ; MU-M ; DUST POLARIZATION ; SCUBA-2 ; OMC-1 ; STRENGTH ; I. ; POLARIMETER ; COMPONENTS |
| Funding Project | National Natural Science Foundation of China (NSFC)[12425304] ; National Natural Science Foundation of China (NSFC)[U1731237] ; National Key R&D Program of China[2017YFA0402700] ; National Key R&D Program of China[2023YFA1608204] ; National Key R&D Program of China[2022YFA1603103] ; China Manned Space Project[CMS-CSST-2021-B06] ; NRC Canada ; NSERC Discovery Grant ; Basic Science Research Program through the NRF - Ministry of Education, Science and Technology[NRF- 2019R1A2C1010851] ; Korea Astronomy and Space Science Institute - Korea government (MSIT)[2024-1-841-00] ; National Research Foundation of Korea (NRF) - Korea government (MSIT)[RS-2024-00342488] ; National Science and Technology Council of Taiwan[109-2112-M-007-010-MY3] ; National Science and Technology Council of Taiwan[112-2112-M-007-011] ; National Science and Technology Council of Taiwan[113-2112-M-007-004] ; international Gemini Observatory, a program of NSF NOIRLab ; U.S. National Science Foundation ; Science and Engineering Research Board (SERB)[RJF/2020/000071] ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; [URF\R1\211322] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001492149500001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | National Natural Science Foundation of China (NSFC) ; National Key R&D Program of China ; China Manned Space Project ; NRC Canada ; NSERC Discovery Grant ; Basic Science Research Program through the NRF - Ministry of Education, Science and Technology ; Korea Astronomy and Space Science Institute - Korea government (MSIT) ; National Research Foundation of Korea (NRF) - Korea government (MSIT) ; National Science and Technology Council of Taiwan ; international Gemini Observatory, a program of NSF NOIRLab ; U.S. National Science Foundation ; Science and Engineering Research Board (SERB) ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/7781 |
| Collection | 射电天文研究室_恒星形成与演化研究团组 |
| Corresponding Author | Qiu, Keping |
| Affiliation | 1.Nanjing Univ, Sch Astron & Space Sci, 163 Xianlin Ave, Nanjing 210023, Jiangsu, Peoples R China 2.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Jiangsu, Peoples R China 3.Inst Astrofis Canarias, E-38205 Tenerife, Canary Islands, Spain 4.Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain 5.Univ Montreal, Ctr Rech Astrophys Quebec, 1375 Ave Therese Lavoie Roux, Montreal, PQ H2V OB3, Canada 6.Univ Montreal, Dept Phys, 1375 Ave Therese Lavoie Roux, Montreal, PQ H2V OB3, Canada 7.Natl Astron Observ Japan, Div ALMA, Mitaka, Tokyo 1818588, Japan 8.Natl Radio Astron Observ, 1003 Lopezville Rd, Socorro, NM 87801 USA 9.Jodrell Bank, SKA Observ, Macclesfield SK11 9FT, Cheshire, England 10.Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England 11.Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England 12.UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England 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F-91191 Gif Sur Yvette, France 100.Jet Prop Lab, MS 169-506,4800 Oak Grove Dr, Pasadena, CA 91109 USA 101.Univ South Wales, Pontypridd CF37 1DL, M Glam, Wales 102.Univ Leeds, Dept Appl Math, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England 103.Univ Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France 104.Univ Leeds, Sch Phys & Astron, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England |
| Recommended Citation GB/T 7714 | Wu, Jintai,Qiu, Keping,Poidevin, Frederick,et al. A Tale of Three: Magnetic Fields along the Orion Integral-shaped Filament as Revealed by the JCMT BISTRO Survey[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,977(2):14. |
| APA | Wu, Jintai.,Qiu, Keping.,Poidevin, Frederick.,Bastien, Pierre.,Liu, Junhao.,...&van Loo, Sven.(2024).A Tale of Three: Magnetic Fields along the Orion Integral-shaped Filament as Revealed by the JCMT BISTRO Survey.ASTROPHYSICAL JOURNAL LETTERS,977(2),14. |
| MLA | Wu, Jintai,et al."A Tale of Three: Magnetic Fields along the Orion Integral-shaped Filament as Revealed by the JCMT BISTRO Survey".ASTROPHYSICAL JOURNAL LETTERS 977.2(2024):14. |
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