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Record W4312070186 · doi:10.3847/1538-4357/ac9dfb

The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament

2022· article· en· W4312070186 on OpenAlexafffund
Tao-Chung Ching, Keping Qiu, Di Li, Zhiyuan Ren, S. Lai, David Berry, Kate Pattle, Ray S. Furuya, D. Ward–Thompson, Doug Johnstone, Patrick M. Koch, Chang Won Lee, Thiem Hoang, Tetsuo Hasegawa, Woojin Kwon, Pierre Bastien, Chakali Eswaraiah, Jia-Wei Wang, Kyoung Hee Kim, Jihye Hwang, Archana Soam, A-Ran Lyo, Junhao Liu, Valentin J. M. Le Gouellec, D. Arzoumanian, A. P. Whitworth, James Di Francesco, F. Poidevin, Tie Liu, Simon Coudé, Mehrnoosh Tahani, Hongli Liu, Takashi Onaka, Motohide Tamura, Zhiwei Chen, Xindi Tang, Florian Kirchschlager, Tyler L. Bourke, Do‐Young Byun, Mike Chen, Huei-Ru Vivien Chen, Wen-Ping Chen, Jungyeon Cho, Yunhee Choi, Young-Woo Choi, Minho Choi, A. Chrysostomou, Eun Jung Chung, Y. Sophia Dai, Pham Ngoc Diep, Yasuo Doi, Yan Duan, Hao-Yuan Duan, David Eden, Lapo Fanciullo, Jason Fiege, Laura M. Fissel, Erica Franzmann, Per Friberg, Rachel Friesen, G. A. Fuller, T. M. Gledhill, Sarah Graves, J. S. Greaves, Matt Griffin, Qilao Gu, Ilseung Han, Saeko S. Hayashi, Martin Houde, Charles L. H. Hull, Tsuyoshi Inoue, Shu‐ichiro Inutsuka, Kazunari Iwasaki, Il-Gyo Jeong, V. Könyves, Ji‐hyun Kang, Miju Kang, Janik Karoly, Akimasa Kataoka, Koji S. Kawabata, F. Kemper, Jongsoo Kim, Mi-Ryang Kim, Shinyoung Kim, Hyosung Kim, Kee‐Tae Kim, Gwanjeong Kim, J. M. Kirk, Masato I. N. Kobayashi, Takayoshi Kusune, Jungmi Kwon, Kevin Lacaille, Chi-Yan Law, Sang-Sung Lee, Hyeseung Lee, Jeong‐Eun Lee, Chin‐Fei Lee, Yong-Hee Lee, Guang-Xing Li, Hua-bai Li, Sheng-Jun Lin, Sheng‐Yuan Liu, Xing Lu, Steve Mairs, M. Matsumura, Brenda C. Matthews, G. H. Moriarty‐Schieven, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nguyen Bich Ngoc, Nagayoshi Ohashi, Geumsook Park, Harriet Parsons, N. Peretto, F D Priestley, Tae‐Soo Pyo, Lei Qian, Ramprasad Rao, Mark G. Rawlings, J. M. C. Rawlings, Brendan Retter, John Richer, A. J. Rigby, Sarah Sadavoy, Hiro Saito, G. Savini, Masumichi Seta, Yoshito Shimajiri, Hiroko Shinnaga, Ya‐Wen Tang, Kohji Tomisaka, Le Ngoc Tram, Yusuke Tsukamoto, S. Viti, Hongchi Wang, Jintai Wu, Jinjin Xie, Meng-Zhe Yang, Hsi-Wei Yen, Hyunju Yoo, Jinghua Yuan, Hyeong-Sik Yun, Tetsuya Zenko, Chuan-Peng Zhang, Yapeng Zhang, Guoyin Zhang, Jianjun Zhou, Ilse De Looze, P. André, C. D. Dowell, S. P. S. Eyres, S. A. E. G. Falle, Jean‐François Robitaille, S. Van Loo

Bibliographic record

VenueThe Astrophysical Journal · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsDalhousie UniversityWestern UniversityMcMaster UniversityQueen's UniversityUniversity of ManitobaUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of VictoriaHerzberg Institute of Astrophysics
FundersAgencia Estatal de InvestigaciónScience and Engineering Research BoardJapan Society for the Promotion of ScienceNatural Sciences and Engineering Research Council of CanadaMinistry of Science and ICT, South KoreaNational Astronomical Observatory of JapanMinistry of Science and Technology, TaiwanNational Research Foundation of KoreaMinistry of Education, Science and TechnologyKorea Astronomy and Space Science InstituteChinese Academy of SciencesDepartment of Science and Technology, Ministry of Science and Technology, IndiaNational Natural Science Foundation of ChinaAcademia SinicaScience and Technology Facilities CouncilNational Research Foundation
KeywordsPhysicsJames Clerk Maxwell TelescopeProtein filamentMagnetic fieldAstrophysicsPolarization (electrochemistry)Star formationGalaxy

Abstract

fetched live from OpenAlex

Abstract We present 850 μm dust polarization observations of the massive DR21 filament from the B-fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter and the SCUBA-2 camera on the James Clerk Maxwell Telescope. We detect ordered magnetic fields perpendicular to the parsec-scale ridge of the DR21 main filament. In the subfilaments, the magnetic fields are mainly parallel to the filamentary structures and smoothly connect to the magnetic fields of the main filament. We compare the POL-2 and Planck dust polarization observations to study the magnetic field structures of the DR21 filament on 0.1–10 pc scales. The magnetic fields revealed in the Planck data are well-aligned with those of the POL-2 data, indicating a smooth variation of magnetic fields from large to small scales. The plane-of-sky magnetic field strengths derived from angular dispersion functions of dust polarization are 0.6–1.0 mG in the DR21 filament and ∼0.1 mG in the surrounding ambient gas. The mass-to-flux ratios are found to be magnetically supercritical in the filament and slightly subcritical to nearly critical in the ambient gas. The alignment between column density structures and magnetic fields changes from random alignment in the low-density ambient gas probed by Planck to mostly perpendicular in the high-density main filament probed by James Clerk Maxwell Telescope. The magnetic field structures of the DR21 filament are in agreement with MHD simulations of a strongly magnetized medium, suggesting that magnetic fields play an important role in shaping the DR21 main filament and subfilaments.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.005
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.010
GPT teacher head0.223
Teacher spread0.213 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations24
Published2022
Admission routes2
Has abstractyes

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