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The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333
Doi, Yasuo1; Hasegawa, Tetsuo2; Furuya, Ray S.3; Coude, Simon4,5; Hull, Charles L. H.6,7; Arzoumanian, Doris8,9; Bastien, Pierre5,10; Chen, Michael Chun-Yuan11; Di Francesco, James11,12; Friesen, Rachel13; Houde, Martin14; Inutsuka, Shu-ichiro9; Mairs, Steve15; Matsumura, Masafumi16; Onaka, Takashi17,18; Sadavoy, Sarah19; Shimajiri, Yoshito2,20; Tahani, Mehrnoosh21; Tomisaka, Kohji22,23; Eswaraiah, Chakali24,25; Koch, Patrick M.26; Pattle, Kate27; Lee, Chang Won28,29; Tamura, Motohide17,30; Berry, David15; Ching, Tao-Chung24,25; Hwang, Jihye28,29; Kwon, Woojin28,31; Soam, Archana4,28; Wang, Jia-Wei26; Lai, Shih-Ping26,32; Qiu, Keping33,34; Ward-Thompson, Derek35; Byun, Do-Young28,29; Chen, Huei-Ru Vivien26,32; Chen, Wen Ping36; Chen, Zhiwei37; Cho, Jungyeon38; Choi, Minho28; Choi, Yunhee28; Chrysostomou, Antonio39; Chung, Eun Jung38; Diep, Pham Ngoc40; Duan, Hao-Yuan32; Fanciullo, Lapo26; Fiege, Jason41; Franzmann, Erica41; Friberg, Per15; Fuller, Gary42; Gledhill, Tim39; Graves, Sarah F.15; Greaves, Jane S.43; Griffin, Matt J.43; Gu, Qilao44; Han, Ilseung28,29; Hatchell, Jennifer45; Hayashi, Saeko S.46; Hoang, Thiem28,29; Inoue, Tsuyoshi9; Iwasaki, Kazunari47; Jeong, Il-Gyo28; Johnstone, Doug11,12; Kanamori, Yoshihiro1; Kang, Ji-hyun28; Kang, Miju28; Kang, Sung-ju28; Kataoka, Akimasa22; Kawabata, Koji S.48,49,50; Kemper, Francisca26,51; Kim, Gwanjeong52; Kim, Jongsoo28,29; Kim, Kee-Tae28; Kim, Kyoung Hee28; Kim, Mi-Ryang28; Kim, Shinyoung28,29; Kirk, Jason M.35; Kobayashi, Masato I. N.53; Konyves, Vera35; Kusune, Takayoshi22; Kwon, Jungmi17; Lacaille, Kevin54,55; Law, Chi-Yan44,56; Lee, Chin-Fei26; Lee, Hyeseung38; Lee, Jeong-Eun57; Lee, Sang-Sung28,29; Lee, Yong-Hee15,57; Li, Dalei58; Li, Di24,59; Li, Hua-bai44; Liu, Hong-Li44,60; Liu, Junhao33,34; Liu, Sheng-Yuan26; Liu, Tie61; de Looze, Ilse62; Lyo, A-Ran28; Matthews, Brenda C.11,12; Moriarty-Schieven, Gerald H.12; Nagata, Tetsuya63; Nakamura, Fumitaka22,23; Nakanishi, Hiroyuki20; Ohashi, Nagayoshi26; Park, Geumsook28; Parsons, Harriet15; Peretto, Nicolas43; Pyo, Tae-Soo23,46; Qian, Lei24; Rao, Ramprasad26; Rawlings, Mark G.15; Retter, Brendan43; Richer, John64,65; Rigby, Andrew43; Saito, Hiro66; Savini, Giorgio62; Scaife, Anna M. M.42; Seta, Masumichi67; Shinnaga, Hiroko20; Tang, Ya-Wen26; Tsukamoto, Yusuke20; Viti, Serena62; Wang, Hongchi37; Whitworth, Anthony P.43; Yen, Hsi-Wei26; Yoo, Hyunju28; Yuan, Jinghua25; Yun, Hyeong-Sik57; Zenko, Tetsuya63; Zhang, Chuan-Peng24,25; Zhang, Guoyin24; Zhang, Yapeng44; Zhou, Jianjun58; Zhu, Lei24; Andre, Philippe68; Dowell, C. Darren69; Eyres, Stewart P. S.35; Falle, Sam70; van Loo, Sven71; Robitaille, Jean-Francois72
2020-08-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume899Issue:1Pages:28
Contribution Rank58
AbstractWe present new observations of the active star formation region NGC 1333 in the Perseus molecular cloud complex from the James Clerk Maxwell TelescopeB-Fields In Star-forming Region Observations (BISTRO) survey with the POL-2 instrument. The BISTRO data cover the entire NGC 1333 complex (similar to 1.5 pc x 2 pc) at 0.02 pc resolution and spatially resolve the polarized emission from individual filamentary structures for the first time. The inferred magnetic field structure is complex as a whole, with each individual filament aligned at different position angles relative to the local field orientation. We combine the BISTRO data with low- and high- resolution data derived from Planck and interferometers to study the multiscale magnetic field structure in this region. The magnetic field morphology drastically changes below a scale of similar to 1 pc and remains continuous from the scales of filaments (similar to 0.1 pc) to that of protostellar envelopes (similar to 0.005 pc or similar to 1000 au). Finally, we construct simple models in which we assume that the magnetic field is always perpendicular to the long axis of the filaments. We demonstrate that the observed variation of the relative orientation between the filament axes and the magnetic field angles are well reproduced by this model, taking into account the projection effects of the magnetic field and filaments relative to the plane of the sky. These projection effects may explain the apparent complexity of the magnetic field structure observed at the resolution of BISTRO data toward the filament network.
KeywordInterstellar medium Interstellar magnetic fields Interstellar filaments Star formation Polarimetry Submillimeter astronomy
DOI10.3847/1538-4357/aba1e2
URL查看原文
Indexed BySCI
Language英语
WOS KeywordLARGE-SCALE STRUCTURE ; RADIATIVE TORQUES ; STAR-FORMATION ; MOLECULAR CLOUD ; INTERSTELLAR GRAINS ; PERSEUS ; TAURUS ; SCUBA-2 ; SUBMILLIMETER ; ALIGNMENT
Funding ProjectNational Key R&D Program of China[2017YFA0402700] ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canadian Space Agency ; Japan Society for the Promotion of Science[25247016] ; Japan Society for the Promotion of Science[18H01250] ; Japan Society for the Promotion of Science[19H01938] ; Universities Space Research Association ; National Aeronautics and Space administration[NNA17BF53C] ; NAOJ Fellowship ; JSPS KAKENHI[18K13586] ; FCT/MCTES through national funds (PIDDAC)[UID/FIS/04434/2019] ; Ministry of Science and Technology of Taiwan[MoST107-2119-M-001-031-MY3] ; Academia Sinica[AS-IA-106-M03] ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology[NRF-2019R1A2C1010851] ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Science, ICT & Future Planning[NRF-2015R1C1A1A01052160] ; NSFC[11725313] ; Seoul National University ; Basic Science Research Program through the National Research Foundation of Korea[NRF-2016R1C1B2013642] ; [25]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000561536000001
PublisherIOP PUBLISHING LTD
Funding OrganizationNational Key R&D Program of China ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation ; Canadian Space Agency ; Japan Society for the Promotion of Science ; Universities Space Research Association ; National Aeronautics and Space administration ; NAOJ Fellowship ; JSPS KAKENHI ; FCT/MCTES through national funds (PIDDAC) ; Ministry of Science and Technology of Taiwan ; Academia Sinica ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science and Technology ; Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Science, ICT & Future Planning ; NSFC ; Seoul National University ; Basic Science Research Program through the National Research Foundation of Korea
Citation statistics
Cited Times:13[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3627
Collection射电天文研究室_恒星形成与演化研究团组
Corresponding AuthorDoi, Yasuo
Affiliation1.Univ Tokyo, Grad Sch Arts & Sci, Dept Earth Sci & Astron, Meguro Ku, 3-8-1 Komaba, Tokyo 1538902, Japan
2.Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
3.Tokushima Univ, Inst Liberal Arts & Sci, Minami Jousanajima Machi 1-1, Tokushima 7708502, Japan
4.Univ Space Res Assoc, SOFIA Sci Ctr, NASA, Ames Res Ctr, MS N232-12, Moffett Field, CA 94035 USA
5.Univ Montreal, Dept Phys, Ctr Rech Astrophys Quebec CRAQ, CP 6128 Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada
6.Natl Astron Observ Japan, NAOJ Chile, Alonso de Cordova 3788,Off 61B, Santiago 7630422, Chile
7.Joint Alma Observ, Alonso de Cordova 3107, Santiago, Chile
8.Univ Porto, CAUP, Inst Astrofis & Ciencias Espaco, Rua Estrelas, P-4150762 Porto, Portugal
9.Nagoya Univ, Grad Sch Sci, Dept Phys, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan
10.Univ Montreal, Inst Rech Exoplanetes iREx, Dept Phys, CP 6128 Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada
11.Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
12.Natl Res Council Canada, Herzberg Astron & Astrophys Res Ctr, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada
13.Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA
14.Univ Western Ontario, Dept Phys & Astron, 1151 Richmond St, London, ON N6A 3K7, Canada
15.East Asian Observ, 660 N Aohoku Pl,Univ Pk, Hilo, HI 96720 USA
16.Kagawa Univ, Fac Educ, Saiwai Cho 1-1, Takamatsu, Kagawa 7608522, Japan
17.Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
18.Meisei Univ, Fac Sci & Engn, Dept Phys, 2-1-1 Hodokubo, Hino, Tokyo 1918506, Japan
19.Queens Univ, Dept Phys Engn Phys & Astrophys, Kingston, ON K7L 3N6, Canada
20.Kagoshima Univ, Grad Sch Sci & Engn, Dept Phys & Astron, 1-21-35 Korimoto, Kagoshima, Kagoshima 8900065, Japan
21.Natl Res Council Canada, Herzberg Astron & Astrophys Res Ctr, Dominion Radio Astrophys Observ, POB 248, Penticton, BC V2A 6J9, Canada
22.Natl Astron Observ Japan, Div Theoret Astron, Mitaka, Tokyo 1818588, Japan
23.SOKENDAI Grad Univ Adv Studies, Hayama, Kanagawa 2400193, Japan
24.Chinese Acad Sci, Natl Astron Observ, CAS Key Lab FAST, Beijing, Peoples R China
25.Chinese Acad Sci, Natl Astron Observ, A20 Datun Rd, Beijing 100012, Peoples R China
26.Acad Sinica, Inst Astron & Astrophys, AS NTU, 11F Astron Math Bldg,1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan
27.Natl Univ Ireland Galway, Ctr Astron, Sch Phys, Univ Rd, Galway, Ireland
28.Korea Astron & Space Sci Inst KASI, 776 Daedeokdae Ro, Daejeon 34055, South Korea
29.Univ Sci & Technol, 217 Gajang Ro, Daejeon 34113, South Korea
30.Natl Inst Nat Sci, Astrobiol Ctr, Mitaka, Tokyo 1818588, Japan
31.Seoul Natl Univ SNU, Dept Earth Sci Educ, 1 Gwanak Ro, Seoul 08826, South Korea
32.Natl Tsing Hua Univ, Inst Astron & Dept Phys, Hsinchu 30013, Taiwan
33.Nanjing Univ, Sch Astron & Space Sci, 163 Xianlin Ave, Nanjing 210023, Peoples R China
34.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China
35.Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England
36.Natl Cent Univ, Inst Astron, Chungli 32054, Taiwan
37.Chinese Acad Sci, Purple Mt Observ, 2 West Beijing Rd, Nanjing 210008, Peoples R China
38.Chungnam Natl Univ, Dept Astron & Space Sci, 99 Daehak Ro, Daejeon 34134, South Korea
39.Univ Hertfordshire, Sch Phys Astron & Math, Coll Lane, Hatfield AL10 9AB, Herts, England
40.Vietnam Acad Sci & Technol, Vietnam Natl Space Ctr, 18 Hoang Quoc Viet, Hanoi, Vietnam
41.Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada
42.Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Oxford Rd, Manchester M13 9PL, Lancs, England
43.Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales
44.Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China
45.Univ Exeter, Phys & Astron, Stocker Rd, Exeter EX4 4QL, Devon, England
46.Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA
47.Doshisha Univ, Dept Environm Syst Sci, Miyakodani 1-3, Kyoto 6100394, Japan
48.Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Kagamiyama 1-3-1, Higashihiroshima, Hiroshima 7398526, Japan
49.Hiroshima Univ, Dept Phys, Kagamiyama 1-3-1, Higashihiroshima, Hiroshima 7398526, Japan
50.Hiroshima Univ, Core Res Energet Universe Core, Kagamiyama 1-3-1, Higashihiroshima, Hiroshima 7398526, Japan
51.European Southern Observ ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany
52.Natl Inst Nat Sci, Nobeyama Radio Observ, Natl Astron Observ Japan, Minamisa Ku, Minamimaki, Nagano 3841305, Japan
53.Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, 1-1 Machikaneyama Cho, Toyonaka, Osaka, Japan
54.McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada
55.Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS B3H 4R2, Canada
56.Chalmers Univ Technol, Dept Space Earth & Environm, SE-41296 Gothenburg, Sweden
57.Kyung Hee Univ, Sch Space Res, 1732 Deogyeong Daero, Yongin 17104, Gyeonggi Do, South Korea
58.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
59.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
60.Univ Concepcion, Dept Astron, Av Esteban Iturra S-N,160-C, Concepcion, Chile
61.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
62.UCL, Phys & Astron Dept, London WC1E 6BT, England
63.Kyoto Univ, Grad Sch Sci, Dept Astron, Sakyo Ku, Kyoto 6068502, Japan
64.Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England
65.Univ Cambridge, Kavli Inst Cosmol, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
66.Tokyo Gakugei Univ, Dept Astron & Earth Sci, Koganei, Tokyo 1848501, Japan
67.Kwansei Gakuin Univ, Sch Sci & Technol, Dept Phys, 2-1 Gakuen, Sanda, Hyogo 6691337, Japan
68.Univ Paris Diderot, Lab AIM CEA, CEA Saclay, DSM,CNRS,IRFU,Serv Astrophys, F-91191 Gif Sur Yvette, France
69.Jet Prop Lab, MS 169-506,4800 Oak Grove Dr, Pasadena, CA 91109 USA
70.Univ Leeds, Dept Appl Math, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England
71.Univ Leeds, Sch Phys & Astron, Woodhouse Lane, Leeds LS2 9JT, W Yorkshire, England
72.Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France
Recommended Citation
GB/T 7714
Doi, Yasuo,Hasegawa, Tetsuo,Furuya, Ray S.,et al. The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333[J]. ASTROPHYSICAL JOURNAL,2020,899(1):28.
APA Doi, Yasuo.,Hasegawa, Tetsuo.,Furuya, Ray S..,Coude, Simon.,Hull, Charles L. H..,...&Robitaille, Jean-Francois.(2020).The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333.ASTROPHYSICAL JOURNAL,899(1),28.
MLA Doi, Yasuo,et al."The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333".ASTROPHYSICAL JOURNAL 899.1(2020):28.
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