KMS of Xinjiang Astronomical Observatory, CAS
| Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations | |
Wang, Jia-Wei1; Koch, Patrick M.1; Clarke, Seamus D.1; Fuller, Gary2,3; Peretto, Nicolas4; Tang, Ya-Wen1; Yen, Hsi-Wei1; Lai, Shih-Ping1,5,6; Ohashi, Nagayoshi1; Arzoumanian, Doris7; Johnstone, Doug8,9; Furuya, Ray10; Inutsuka, Shu-ichiro11; Lee, Chang Won12,13; Ward-Thompson, Derek14; Le Gouellec, Valentin J. M.15; Liu, Hong-Li16; Fanciullo, Lapo17; Hwang, Jihye12; Pattle, Kate18; Poidevin, Frederick19,20; Tahani, Mehrnoosh21; Onaka, Takashi22; Rawlings, Mark G.23; Chung, Eun Jung24; Liu, Junhao25; Lyo, A-Ran12; Priestley, Felix4; Hoang, Thiem12,13; Tamura, Motohide22,26,27; Berry, David25; Bastien, Pierre28,29; Ching, Tao-Chung30; Coude, Simon31,32; Kwon, Woojin33,34; Chen, Mike35; Eswaraiah, Chakali36; Soam, Archana37; Hasegawa, Tetsuo26; Qiu, Keping38,39; Bourke, Tyler L.2,40; Byun, Do-Young12,13; Chen, Zhiwei41; Chen, Huei-Ru Vivien1,5,6; Chen, Wen Ping42; Cho, Jungyeon24; Choi, Minho12; Choi, Yunhee12; Choi, Youngwoo43; Chrysostomou, Antonio40; Dai, Sophia44; Di Francesco, James8,9; Diep, Pham Ngoc45; Doi, Yasuo46; Duan, Yan44; Duan, Hao-Yuan42; Eden, David47; Fiege, Jason48; Fissel, Laura M.35; Franzmann, Erica48; Friberg, Per25; Friesen, Rachel49; Gledhill, Tim50; Graves, Sarah25; Greaves, Jane4; Griffin, Matt4; Gu, Qilao51; Han, Ilseung12,13; Hayashi, Saeko52; Houde, Martin53; Inoue, Tsuyoshi54; Iwasaki, Kazunari55; Jeong, Il-Gyo12,56; Koenyves, Vera14; Kang, Ji-hyun12; Kang, Miju12; Karoly, Janik14; Kataoka, Akimasa57; Kawabata, Koji58,59,60; Khan, Zacariyya18; Kim, Mi-Ryang61; Kim, Kee-Tae12,13; Kim, Kyoung Hee62; Kim, Shinyoung12; Kim, Jongsoo12,13; Kim, Hyosung33; Kim, Gwanjeong63; Kirchschlager, Florian64; Kirk, Jason14; Kobayashi, Masato I. N.7; Kusune, Takayoshi65; Kwon, Jungmi22; Lacaille, Kevin66,67; Law, Chi-Yan68,69; Lee, Sang-Sung12,13; Lee, Hyeseung70; Lee, Jeong-Eun71; Lee, Chin-Fei1; Li, Dalei72 ; Li, Hua-bai68; Li, Guangxing73; Li, Di74,75; Lin, Sheng-Jun1; Liu, Tie76; Liu, Sheng-Yuan1; Lu, Xing51; Mairs, Steve25; Matsumura, Masafumi77,78; Matthews, Brenda8,9; Moriarty-Schieven, Gerald8; Nagata, Tetsuya79; Nakamura, Fumitaka57,80; Nakanishi, Hiroyuki81; Ngoc, Nguyen Bich45,82; Park, Geumsook12; Parsons, Harriet25; Pyo, Tae-Soo52,80; Qian, Lei74; Rao, Ramprasad1; Rawlings, Jonathan18; Retter, Brendan4; Richer, John83,84; Rigby, Andrew4; Sadavoy, Sarah35; Saito, Hiro85; Savini, Giorgio86; Seta, Masumichi87; Sharma, Ekta74; Shimajiri, Yoshito88; Shinnaga, Hiroko81; Tang, Xindi89; Thuong, Hoang Duc90; Tomisaka, Kohji57; Tram, Le Ngoc91; Tsukamoto, Yusuke81; Viti, Serena92; Wang, Hongchi41; Whitworth, Anthony4; Wu, Jintai38; Xie, Jinjin44; Yang, Meng-Zhe5,6; Yoo, Hyunju24; Yuan, Jinghua44; Yun, Hyeong-Sik12; Zenko, Tetsuya79; Zhang, Chuan-Peng44,74; Zhang, Yapeng93; Zhang, Guoyin74; Zhou, Jianjun72; Zhu, Lei74; de Looze, Ilse64; Andre, Philippe94; Dowell, C. Darren95; Eyres, Stewart96; Falle, Sam97; Robitaille, Jean-Francois98; van Loo, Sven99
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| 2024-02-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 962Issue:2Pages:136 |
| Contribution Rank | 70 |
| Abstract | We report 850 mu m continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B-fields In STar forming Regions Observations large program on the James Clerk Maxwell Telescope. These data reveal a well-structured nonuniform magnetic field in the NGC 2264C and 2264D regions with a prevailing orientation around 30 degrees from north to east. Field strength estimates and a virial analysis of the major clumps indicate that NGC 2264C is globally dominated by gravity, while in 2264D, magnetic, gravitational, and kinetic energies are roughly balanced. We present an analysis scheme that utilizes the locally resolved magnetic field structures, together with the locally measured gravitational vector field and the extracted filamentary network. From this, we infer statistical trends showing that this network consists of two main groups of filaments oriented approximately perpendicular to one another. Additionally, gravity shows one dominating converging direction that is roughly perpendicular to one of the filament orientations, which is suggestive of mass accretion along this direction. Beyond these statistical trends, we identify two types of filaments. The type I filament is perpendicular to the magnetic field with local gravity transitioning from parallel to perpendicular to the magnetic field from the outside to the filament ridge. The type II filament is parallel to the magnetic field and local gravity. We interpret these two types of filaments as originating from the competition between radial collapsing, driven by filament self-gravity, and longitudinal collapsing, driven by the region's global gravity. |
| DOI | 10.3847/1538-4357/ad165b |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | MOLECULAR CLOUD ; CLUSTER-FORMATION ; SPITZER VIEW ; DUST ; GRAVITY ; CORE ; VELOCITY ; POLARIZATION ; HERSCHEL ; SIMULATIONS |
| Funding Project | National Key R&D Program of China[2017YFA0402700] ; National Key R&D Program of China[2022YFA1603100] ; National Key R&D Program of China[2017YFA0402604] ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; National Science and Technology Council (NSTC) in Taiwan[2017YFA0402700] ; National Science and Technology Council (NSTC) in Taiwan[2022YFA1603100] ; National Science and Technology Council (NSTC) in Taiwan[NSTC 112-2112-M-001-049] ; National Science and Technology Council (NSTC) in Taiwan[NSTC 111-2112-M-001-039] ; National Natural Science Foundation of China (NSFC)[U1731237] ; China Manned Space Project[CMS-CSST-2021-B06] ; Agencia Canaria de Investigacion, Innovacion y Sociedad de la Informacion (ACIISI) under the European FEDER (FONDO EUROPEO DE DESARROLLO REGIONAL) de Canarias[2017YFA0402604] ; Agencia Canaria de Investigacion, Innovacion y Sociedad de la Informacion (ACIISI) under the European FEDER (FONDO EUROPEO DE DESARROLLO REGIONAL) de Canarias[PROID2021010078] ; NOIRLab[NSTC 112-2112-M-001-049] ; Ministry of Science and Technology of Taiwan[NSTC 111-2112-M-001-039] ; Ministry of Science and Technology of Taiwan[111-2811-M-005-007] ; Ministry of Science and Technology of Taiwan[109-2112-M-005-003-MY3] ; NRC Canada[U1731237] ; NSERC Discovery Grant[CMS-CSST-2021-B06] ; Science and Engineering Research Board (SERB), Department of Science and Technology (DST), Government of India[RJF/2020/000071] ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[PROID2021010078] ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[111-2811-M-005-007] ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[NRF- 2019R1A2C1010851] ; Korea Astronomy and Space Science Institute - Korean government (MSIT)[2023-1-84000] ; National Research Foundation of Korea (NRF) - Korean government (MSIT)[109-2112-M-005-003-MY3] ; National Research Foundation of Korea (NRF) - Korean government (MSIT)[NRF-2021R1F1A1061794] ; National Research Foundation of Korea (NRF) - Korean government (MSIT)[URF\R1\211322] ; JSPS KAKENHI[18H05442] |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001164527900001 |
| 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 ; National Science and Technology Council (NSTC) in Taiwan ; National Natural Science Foundation of China (NSFC) ; China Manned Space Project ; Agencia Canaria de Investigacion, Innovacion y Sociedad de la Informacion (ACIISI) under the European FEDER (FONDO EUROPEO DE DESARROLLO REGIONAL) de Canarias ; NOIRLab ; Ministry of Science and Technology of Taiwan ; NRC Canada ; NSERC Discovery Grant ; Science and Engineering Research Board (SERB), Department of Science and Technology (DST), Government of India ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology ; Korea Astronomy and Space Science Institute - Korean government (MSIT) ; National Research Foundation of Korea (NRF) - Korean government (MSIT) ; JSPS KAKENHI |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5857 |
| Collection | 中国科学院新疆天文台 |
| Corresponding Author | Wang, Jia-Wei |
| Affiliation | 1.Acad Sinica, Inst Astron & Astrophys, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan 2.Univ Manchester, Sch Phys & Astron, Ctr Astrophys, Jodrell Bank, Oxford Rd, Manchester M13 9PL, Lancs, England 3.Univ Cologne, Phys Inst, Zulpicher Str 77, D-50937 Cologne, Germany 4.Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales 5.Natl Tsing Hua Univ, Inst Astron, Hsinchu 30013, Taiwan 6.Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan 7.Natl Astron Observ Japan, Div Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 8.NRC Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada 9.Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada 10.Tokushima Univ, Inst Liberal Arts & Sci, Minami Jousanajima Machi 1-1, Tokushima 7708502, Japan 11.Nagoya Univ, Grad Sch Sci, Dept Phys, Furo Cho,Chikusa Ku, Nagoya, Aichi 4648602, Japan 12.Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea 13.Univ Sci & Technol, 217 Gajeong Ro, 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F-38000 Grenoble, France 99.Univ Leeds, Sch Phys & Astron, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England |
| Recommended Citation GB/T 7714 | Wang, Jia-Wei,Koch, Patrick M.,Clarke, Seamus D.,et al. Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations[J]. ASTROPHYSICAL JOURNAL,2024,962(2):136. |
| APA | Wang, Jia-Wei.,Koch, Patrick M..,Clarke, Seamus D..,Fuller, Gary.,Peretto, Nicolas.,...&van Loo, Sven.(2024).Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations.ASTROPHYSICAL JOURNAL,962(2),136. |
| MLA | Wang, Jia-Wei,et al."Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations".ASTROPHYSICAL JOURNAL 962.2(2024):136. |
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