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Record W2950731126 · doi:10.48550/arxiv.1904.07221

The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region

2019· article· en· W2950731126 on OpenAlex
Simon Coudé, Pierre Bastien, Martin Houde, Sarah Sadavoy, Rachel Friesen, James Di Francesco, Doug Johnstone, Steve Mairs, Tetsuo Hasegawa, Woojin Kwon, Keping Qiu, D. Ward–Thompson, David Berry, Michael Chun-Yuan Chen, Jason Fiege, Erica Franzmann, J. Hatchell, Kevin Lacaille, Brenda C. Matthews, G. H. Moriarty‐Schieven, Andy Pon, P. André, D. Arzoumanian, Yusuke Aso, Chakali Eswaraiah, Jungyeon Cho, Minho Choi, A. Chrysostomou, Eun Jung Chung, Yasuo Doi, E. Drabek-Maunder, C. D. Dowell, S. P. S. Eyres, S. A. E. G. Falle, Per Friberg, G. A. Fuller, Ray S. Furuya, T. M. Gledhill, Sarah Graves, J. S. Greaves, M. J. Griffin, Qilao Gu, Saeko S. Hayashi, Thiem Hoang, W. S. Holland, Tsuyoshi Inoue, Kazunari Iwasaki, Yoshihiro Kanamori, Akimasa Kataoka, Miju Kang, Koji S. Kawabata, F. Kemper, Gwanjeong Kim, Jongsoo Kim, Kyoung Hee Kim, Shinyoung Kim, J. M. Kirk, Masato I. N. Kobayashi, Patrick M. Koch, Jungmi Kwon, Chang Won Lee, Di Li, Hongli Liu, Junhao Liu, Tie Liu, S. Van Loo, M. Matsumura, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nagayoshi Ohashi, Takashi Onaka, Harriet Parsons, Kate Pattle, N. Peretto, Lei Qian, Ramprasad Rao, Mark G. Rawlings, Brendan Retter, John Richer, A. J. Rigby, Hiro Saito, G. Savini, Anna M. M. Scaife, Masumichi Seta, Hiroko Shinnaga, Archana Soam, Motohide Tamura, Kohji Tomisaka, Yusuke Tsukamoto, Hongchi Wang, A. P. Whitworth, Hyunju Yoo, Jinghua Yuan, Tetsuya Zenko, Guoyin Zhang, Jianjun Zhou

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.
fundA Canadian funder is recorded on the work.

Bibliographic record

VenueWhite Rose Research Online (University of Leeds, The University of Sheffield, University of York) · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsMcMaster UniversityDalhousie UniversityUniversity of ManitobaHerzberg Institute of AstrophysicsNational Research Council CanadaWestern UniversityUniversity of VictoriaUniversité de MontréalCentre for Research in Astrophysics of Québec
FundersNational Key Research and Development Program of ChinaNational Research FoundationScience and Technology Facilities CouncilNational Astronomical Observatory of JapanNational Research Foundation of KoreaNational Aeronautics and Space AdministrationMinistry of Education, Science and TechnologyKorea Astronomy and Space Science InstituteUniversities Space Research AssociationNational Natural Science Foundation of ChinaCanadian Space AgencyAcademia Sinica
KeywordsPhysicsMagnetic fieldMolecular cloudSkyPolarization (electrochemistry)AstrophysicsJames Clerk Maxwell TelescopeTurbulenceCosmic microwave backgroundStar formationStarsOpticsMeteorologyChemistry

Abstract

fetched live from OpenAlex

We present the POL-2 850 $μ$m linear polarization map of the Barnard 1 clump in the Perseus molecular cloud complex from the B-fields In STar-forming Region Observations (BISTRO) survey at the James Clerk Maxwell Telescope. We find a trend of decreasing polarization fraction as a function of total intensity, which we link to depolarization effects towards higher density regions of the cloud. We then use the polarization data at 850 $μ$m to infer the plane-of-sky orientation of the large-scale magnetic field in Barnard 1. This magnetic field runs North-South across most of the cloud, with the exception of B1-c where it turns more East-West. From the dispersion of polarization angles, we calculate a turbulence correlation length of $5.0 \pm 2.5$ arcsec ($1500$ au), and a turbulent-to-total magnetic energy ratio of $0.5 \pm 0.3$ inside the cloud. We combine this turbulent-to-total magnetic energy ratio with observations of NH$_3$ molecular lines from the Green Bank Ammonia Survey (GAS) to estimate the strength of the plane-of-sky component of the magnetic field through the Davis-Chandrasekhar-Fermi method. With a plane-of-sky amplitude of $120 \pm 60$ $μ$G and a criticality criterion $λ_c = 3.0 \pm 1.5$, we find that Barnard 1 is a supercritical molecular cloud with a magnetic field nearly dominated by its turbulent component.

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.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Qualitative · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.547
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.001
Science and technology studies0.0020.002
Scholarly communication0.0000.000
Open science0.0020.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

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 head0.026
GPT teacher head0.242
Teacher spread0.215 · 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