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| The JCMT BISTRO-3 Survey: Variation of Magnetic Field Orientations on Parsec and Subparsec Scales in the Massive Star-forming Region G28.34+0.06 | |
Hwang, Jihye1,2,3; Pattle, Kate4; Lee, Chang Won1,5; Karoly, Janik4; Kim, Kee-Tae1,5; Kim, Jongsoo1; Liu, Junhao6; Qiu, Keping7,8; Lyo, A-Ran1; Eden, David9,10; Koch, Patrick M.11; Arzoumanian, Doris2,3,12; Sharma, Ekta13; Poidevin, Frederick14,15; Johnstone, Doug16,17; Coude, Simon18,19; Tahani, Mehrnoosh20; Ward-Thompson, Derek21; Soam, Archana22; Kang, Ji-Hyun1; Hoang, Thiem1,5; Kwon, Woojin23,24,25; Ngoc, Nguyen Bich26,27; Chung, Eun Jung1; Bourke, Tyler L.28,29; Onaka, Takashi30; Kirchschlager, Florian31; Tamura, Motohide30,32,33; Kwon, Jungmi30; Tang, Xindi34 ; Chakali, Eswaraiah35,36; Liu, Tie37; Bastien, Pierre38,39; Furuya, Ray S.40,41; Lai, Shih-Ping11,42,43; Lin, Sheng-Jun11; Wang, Jia-Wei44; Berry, David44
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| 2025-06-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 985Issue:2Pages:222 |
| Contribution Rank | 34 |
| Abstract | Magnetic fields play a significant role in star-forming processes on core to clump scales. We investigate magnetic field orientations and strengths in the massive star-forming clump P2 within the filamentary infrared dark cloud G28.34+0.06 using dust polarization observations made using SCUBA-2/POL-2 on the James Clerk Maxwell Telescope (JCMT) as part of the B-field In STar-forming Region Observations (or BISTRO) survey. We compare the magnetic field orientations at the clump scale of similar to 2 pc from these JCMT observations with those at the core scale of similar to 0.2 pc from archival Atacama Large Millimeter/submillimeter Array data, finding that the magnetic field orientations on these two different scales are perpendicular to one another. We estimate the distribution of magnetic field strengths, which range from 50 to 430 mu G over the clump. The region forming the core shows the highest magnetic field strength. We also obtain the distribution of mass-to-flux ratios across the clump. In the region surrounding the core, the mass-to-flux ratio is larger than 1, which indicates that the magnetic field strength is insufficient to support the region against gravitational collapse. Therefore, the change in the magnetic field orientation from clump to core scales may be the result of gravitational collapse, with the field being pulled inward along with the flow of material under gravity. |
| DOI | 10.3847/1538-4357/adce80 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | SCUBA-2 ; CLOUDS ; POLARIZATION ; STRENGTH ; GRAVITY ; LINE |
| Funding Project | Korea Astronomy and Space Science Institute ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China ; Science and Technology Facilities Council of the United Kingdom ; Canada Foundation for Innovation |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001497251100001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | Korea Astronomy and Space Science Institute ; Operation, Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments ; Ministry of Finance of China ; 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/45760611-7/7796 |
| Collection | 射电天文研究室_恒星形成与演化研究团组 |
| Corresponding Author | Hwang, Jihye |
| Affiliation | 1.Korea Astron & Space Sci Inst KASI, 776 Daedeokdae Ro, Daejeon 34055, South Korea 2.Kyushu Univ, Inst Adv Study, Fukuoka, Japan 3.Kyushu Univ, Fac Sci, Dept Earth & Planetary Sci, Nishi Ku, Fukuoka 8190395, Japan 4.UCL, Dept Phys & Astron, London WC1E 6BT, England 5.Univ Sci & Technol Korea UST, 217 Gajeong Ro, Daejeon 34113, South Korea 6.Natl Astron Observ Japan, Div ALMA, Mitaka, Tokyo 1818588, Japan 7.Nanjing Univ, Sch Astron & Space Sci, 163 Xianlin Ave, Nanjing 210023, Peoples R China 8.Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210023, Peoples R China 9.Univ Bath, Dept Phys, Bath BA2 7AY, England 10.Armagh Observ & Planetarium, Coll Hill, Armagh BT61 9DB, North Ireland 11.Acad Sinica, Inst Astron & Astrophys, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan 12.Natl Astron Observ Japan, Div Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 13.Chinese Acad Sci, CAS Key Lab FAST, Natl Astron Observ, Beijing, Peoples R China 14.Inst Astrofisica Canarias, E-38205 Tenerife, Canarias Island, Spain 15.Univ La Laguna ULL, Dept Astrofis, E-38206 San Cristobal la Laguna, Tenerife, Spain 16.NRC Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada 17.Univ Victoria, Dept Phys & Astron, Victoria, BC V8W 2Y2, Canada 18.Worcester State Univ, Dept Earth Environm & Phys, Worcester, MA 01602 USA 19.Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA 20.Stanford Univ, Kavli Inst Particle Astrophys & Cosmol KIPAC, Stanford, CA 94305 USA 21.Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, England 22.Indian Inst Astrophys, 2 Block, Bengaluru 560034, India 23.Seoul Natl Univ, Dept Earth Sci Educ, 1 Gwanak Ro, Seoul 08826, South Korea 24.Seoul Natl Univ, SNU Astron Res Ctr, 1 Gwanak Rro, Seoul 08826, South Korea 25.Seoul Natl Univ, Ctr Educ Res, 1 Gwanak Ro, Seoul 08826, South Korea 26.Vietnam Acad Sci & Technol, Vietnam Natl Space Ctr, 18 Hoang Quoc Viet, Hanoi, Vietnam 27.Vietnam Acad Sci & Technol, Grad Univ Sci & Technol, 18 Hoang Quoc Viet, Hanoi, Vietnam 28.Jodrell Bank, SKA Observ, Macclesfield SK11 9FT, England 29.Univ Manchester, Jodrell Bank, Sch Phys & Astron, Ctr Astrophys, Oxford Rd, Manchester M13 9PL, England 30.Univ Tokyo, Grad Sch Sci, Dept Astron, 7-3-1 Hongo,Bunkyo Ku, Tokyo 1130033, Japan 31.Univ Ghent, Sterrenkundig Observ, Krijgslaan 281-S9, B-9000 Ghent, Belgium 32.Astrobiol Ctr, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 33.Natl Astron Observ, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 34.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 35.Indian Inst Sci Educ & Res IISER Mohali, Dept Phys Sci, Sect 81, Sas Nagar 140306, Punjab, India 36.Indian Inst Sci Educ & Res Tirupati, Dept Phys, Tirupati 517619, Andhra Prades, India 37.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China 38.Univ Montreal, Ctr Rech Astrophys Quebec, CP 6128 Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada 39.Univ Montreal, Dept Phys, CP 6128 Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada 40.Tokushima Univ, Inst Liberal Arts & Sci, Minami Jousanajima Machi 1-1, Tokushima 7708502, Japan 41.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan 42.Natl Tsing Hua Univ, Inst Astron, Hsinchu 30013, Taiwan 43.Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan 44.East Asian Observ, 660 N Aohoku Pl,Univ Pk, Hilo, HI 96720 USA |
| Recommended Citation GB/T 7714 | Hwang, Jihye,Pattle, Kate,Lee, Chang Won,et al. The JCMT BISTRO-3 Survey: Variation of Magnetic Field Orientations on Parsec and Subparsec Scales in the Massive Star-forming Region G28.34+0.06[J]. ASTROPHYSICAL JOURNAL,2025,985(2):222. |
| APA | Hwang, Jihye.,Pattle, Kate.,Lee, Chang Won.,Karoly, Janik.,Kim, Kee-Tae.,...&Berry, David.(2025).The JCMT BISTRO-3 Survey: Variation of Magnetic Field Orientations on Parsec and Subparsec Scales in the Massive Star-forming Region G28.34+0.06.ASTROPHYSICAL JOURNAL,985(2),222. |
| MLA | Hwang, Jihye,et al."The JCMT BISTRO-3 Survey: Variation of Magnetic Field Orientations on Parsec and Subparsec Scales in the Massive Star-forming Region G28.34+0.06".ASTROPHYSICAL JOURNAL 985.2(2025):222. |
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| Hwang-2025-The JCMT （1061KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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