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Record W4321503464 · doi:10.3847/1538-4357/acac81

JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334

2023· article· en· W4321503464 on OpenAlexaff
Mehrnoosh Tahani, Pierre Bastien, Ray S. Furuya, Kate Pattle, Doug Johnstone, D. Arzoumanian, Yasuo Doi, Tetsuo Hasegawa, Shu‐ichiro Inutsuka, Simon Coudé, Laura Fissel, Michael Chun-Yuan Chen, F. Poidevin, Sarah Sadavoy, Rachel Friesen, Patrick M. Koch, James Di Francesco, G. H. Moriarty‐Schieven, Zhiwei Chen, Eun Jung Chung, Chakali Eswaraiah, Lapo Fanciullo, T. M. Gledhill, Valentin J. M. Le Gouellec, Thiem Hoang, Jihye Hwang, Ji‐hyun Kang, Kyoung Hee Kim, Florian Kirchschlager, Woojin Kwon, Chang Won Lee, Hongli Liu, Takashi Onaka, Mark G. Rawlings, Archana Soam, Motohide Tamura, Xindi Tang, Kohji Tomisaka, A. P. Whitworth, Jungmi Kwon, D. Hoang, M. P. Redman, David Berry, Tao-Chung Ching, Jia-Wei Wang, S. Lai, Keping Qiu, D. Ward–Thompson, Martin Houde, Do‐Young Byun, Huei-Ru Vivien Chen, Wen-Ping Chen, Jungyeon Cho, Minho Choi, Yunhee Choi, A. Chrysostomou, Pham Ngoc Diep, Hao-Yuan Duan, Jason Fiege, Erica Franzmann, Per Friberg, G. A. Fuller, Sarah Graves, J. S. Greaves, M. J. Griffin, Qilao Gu, Ilseung Han, J. Hatchell, Saeko S. Hayashi, Charles L. H. Hull, Tsuyoshi Inoue, Kazunari Iwasaki, Il-Gyo Jeong, Yoshihiro Kanamori, Miju Kang, Sung-Ju Kang, Akimasa Kataoka, Koji S. Kawabata, F. Kemper, Gwanjeong Kim, Jongsoo Kim, Kee‐Tae Kim, Mi-Ryang Kim, Shinyoung Kim, J. M. Kirk, Masato I. N. Kobayashi, V. Könyves, Takayoshi Kusune, Kevin Lacaille, Chi-Yan Law, Chin‐Fei Lee, Hyeseung Lee, Jeong‐Eun Lee, Sang-Sung Lee, Yong-Hee Lee, Di Li, Hua-bai Li, Junhao Liu, Sheng‐Yuan Liu, Tie Liu, Ilse De Looze, A-Ran Lyo, Steve Mairs, M. Matsumura, Brenda C. Matthews, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nagayoshi Ohashi, Geumsook Park, Harriet Parsons, N. Peretto, Tae‐Soo Pyo, Lei Qian, Ramprasad Rao, Brendan Retter, John Richer, A. J. Rigby, Hiro Saito, G. Savini, Anna M. M. Scaife, Masumichi Seta, Yoshito Shimajiri, Hiroko Shinnaga, Ya‐Wen Tang, Yusuke Tsukamoto, S. Viti, Hongchi Wang, Hsi-Wei Yen, Hyunju Yoo, Jinghua Yuan, Hyeong-Sik Yun, Tetsuya Zenko, Chuan-Peng Zhang, Guoyin Zhang, Yapeng Zhang, Jianjun Zhou, P. André, C. D. Dowell, S. P. S. Eyres, S. A. E. G. Falle, S. Van Loo, Jean‐François Robitaille

Bibliographic record

VenueThe Astrophysical Journal · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsDalhousie UniversityUniversity of ManitobaWestern UniversityMcMaster UniversityQueen's UniversityUniversity of VictoriaUniversité de MontréalCentre for Research in Astrophysics of QuébecHerzberg Institute of Astrophysics
FundersAgencia Estatal de InvestigaciónScience and Engineering Research BoardJapan Society for the Promotion of ScienceNational Research FoundationScience and Technology Facilities CouncilNational Science and Technology CouncilMinistry of Science and ICT, South KoreaMinistry of Science and Technology, TaiwanMinistry of Education, Science and TechnologyKorea Astronomy and Space Science InstituteNational Research Foundation of KoreaEuropean Regional Development FundAcademia SinicaDepartment of Science and Technology, Ministry of Science and Technology, IndiaAgencia Canaria de Investigación, Innovación y Sociedad de la Información
KeywordsPhysicsMorphology (biology)Magnetic fieldAstronomyField (mathematics)Astrophysics

Abstract

fetched live from OpenAlex

Abstract We study the Hii regions associated with the NGC 6334 molecular cloud observed in the submillimeter and taken as part of the B-fields In STar-forming Region Observations Survey. In particular, we investigate the polarization patterns and magnetic field morphologies associated with these Hii regions. Through polarization pattern and pressure calculation analyses, several of these bubbles indicate that the gas and magnetic field lines have been pushed away from the bubble, toward an almost tangential (to the bubble) magnetic field morphology. In the densest part of NGC 6334, where the magnetic field morphology is similar to an hourglass, the polarization observations do not exhibit observable impact from Hii regions. We detect two nested radial polarization patterns in a bubble to the south of NGC 6334 that correspond to the previously observed bipolar structure in this bubble. Finally, using the results of this study, we present steps (incorporating computer vision; circular Hough transform) that can be used in future studies to identify bubbles that have physically impacted magnetic field lines.

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 score0.011
Threshold uncertainty score0.022

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 science0.0000.000
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 head0.021
GPT teacher head0.228
Teacher spread0.207 · 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

Citations23
Published2023
Admission routes1
Has abstractyes

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