MétaCan
Menu
← Back to cohort
Record W4401229062 · doi:10.1093/mnras/stae1829

Relative alignments between magnetic fields, velocity gradients, and dust emission gradients in NGC 1333

2024· article· en· W4401229062 on OpenAlexafffund
Michael Chun-Yuan Chen, Laura M. Fissel, Sarah Sadavoy, Erik Rosolowsky, Yasuo Doi, D. Arzoumanian, Pierre Bastien, Simon Coudé, James Di Francesco, Rachel Friesen, Ray S. Furuya, Jihye Hwang, Shu‐ichiro Inutsuka, Doug Johnstone, Janik Karoly, Jungmi Kwon, Woojin Kwon, Valentin J. M. Le Gouellec, Hongli Liu, Steve Mairs, Takashi Onaka, Kate Pattle, Mark G. Rawlings, Mehrnoosh Tahani, Motohide Tamura, Jia-Wei Wang

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of TorontoUniversity of VictoriaHerzberg Institute of AstrophysicsUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of AlbertaQueen's University
FundersKey ProgrammeJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilMax-Planck-Institut für AstronomieNational Astronomical Research Institute of ThailandNederlandse Organisatie voor Wetenschappelijk OnderzoekKU LeuvenAcademia SinicaNatural Sciences and Engineering Research Council of CanadaNational Astronomical Observatory of JapanQueen's UniversityJapan Society for the Promotion of Science LondonKorea Astronomy and Space Science InstituteNational Science Foundation
KeywordsPhysicsAstrophysicsMagnetohydrodynamicsVelocity gradientMagnetic fieldVelocity dispersionVector fieldGalaxyMechanics

Abstract

fetched live from OpenAlex

ABSTRACT Magnetic fields play an important role in shaping and regulating star formation in molecular clouds. Here, we present one of the first studies examining the relative orientations between magnetic (B) fields and the dust emission, gas column density, and velocity centroid gradients on the 0.02 pc (core) scales, using the BISTRO and VLA+GBT observations of the NGC 1333 star-forming clump. We quantified these relative orientations using the Project Rayleigh Statistic (PRS) and found preferential global parallel alignment between the B field and dust emission gradients, consistent with large-scale studies with Planck. No preferential global alignments, however, are found between the B field and velocity gradients. Local PRS calculated for subregions defined by either dust emission or velocity coherence further revealed that the B field does not preferentially align with dust emission gradients in most emission-defined subregions, except in the warmest ones. The velocity-coherent structures, on the other hand, also showed no preferred B field alignments with velocity gradients, except for one potentially bubble-compressed region. Interestingly, the velocity gradient magnitude in NGC 1333 ubiquitously features prominent ripple-like structures that are indicative of magnetohydrodynamic (MHD) waves. Finally, we found B field alignments with the emission gradients to correlate with dust temperature and anticorrelate with column density, velocity dispersion, and velocity gradient magnitude. The latter two anticorrelations suggest that alignments between gas structures and B fields can be perturbed by physical processes that elevate velocity dispersion and velocity gradients, such as infall, accretions, and MHD waves.

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 score0.026
Threshold uncertainty score0.052

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 head0.009
GPT teacher head0.219
Teacher spread0.210 · 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

Citations2
Published2024
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicAstrophysics and Star Formation Studies→French-language works237,207→