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Record W4413271005 · doi:10.1093/mnras/staf1159

WISDOM Project – XXIV. Giant molecular clouds of the spiral galaxy NGC 5064: high fraction of retrograde rotation

2025· article· en· W4413271005 on OpenAlexaff
Lijie Liu, Frank H. Shu, Martin Bureau, Kyoko Onishi, Timothy A. Davis, Fu-Heng Liang, Woorak Choi, Thomas G. Williams, Anan Lu, Satoru Iguchi

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsMcGill University
FundersNational Institutes of Natural SciencesJet Propulsion LaboratoryNational Science CouncilEuropean School of OncologyNational Astronomical Observatory of JapanDanmarks GrundforskningsfondKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyScience and Technology Facilities CouncilNational Research FoundationSpace Telescope Science InstituteNational Science FoundationU.S. Nuclear Regulatory CommissionEntomological Society of America
KeywordsPhysicsAstrophysicsMolecular cloudSpiral galaxyGalaxyMilky WayGalaxy rotation curveVirial massMillimeterVirial theoremStar formationRotation (mathematics)StarsGalaxy formation and evolutionGeometry

Abstract

fetched live from OpenAlex

ABSTRACT We present high-resolution ($0. 14\,\mathrm{ arcsec}\times 0. 12\,\mathrm{ arcsec}$ or $31\times 25$ pc$^2$) Atacama Large Millimeter/sub-millimeter Array $^{12}$CO(J = 2–1) observations of the spiral galaxy NGC 5064. Our study identifies 478 molecular clouds, of which 387 are resolved both spatially and spectrally. These clouds exhibit similarities to those of the Milky Way in terms of their sizes, molecular gas masses, velocity dispersions, velocity gradients, and Larson relations. However, the NGC 5064 clouds stand out with slightly higher gas mass surface densities, lower virial parameters ($\langle \alpha _{\rm vir}\rangle =0.48\pm 0.03$ assuming a standard conversion factor $X_{\rm CO}=2\times 10^{20}$ cm$^{-2}$ (K km s$^{-1})^{-1}$; $\alpha _{\rm vir} = 1$ for a lower conversion factor of $X_{\rm CO}=0.96\pm 0.02\times 10^{20}$ cm$^{-2}$ (K km s$^{-1})^{-1}$), and an unusually high fraction of retrograde rotation ($f_{\rm retro}\approx 67~{{\ \rm per\ cent}}$). Retrograde clouds are 18 per cent larger, 58 per cent more massive, 15 per cent more turbulent and have 17 per cent larger gas mass surface densities than prograde clouds. The velocity gradients in the clouds seem to arise from turbulence rather than cloud’s intrinsic rotation or large-scale galaxy rotation. Cloud–cloud collisions provide the most plausible explanation for the elevated retrograde fraction, though further investigation is needed to confirm this scenario. Projection effects due to the galaxy’s high inclination ($i = 70{_{.}^{\circ}} 8$) may further enhance the apparent retrograde fraction. Confirmation using less inclined systems is essential to determine whether the observed dominance of retrograde rotation reflects a genuine physical phenomenon or is significantly shaped by projection effects.

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)0.001
metaresearch head score (Gemma)0.001
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.022
Threshold uncertainty score0.073

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0220.010

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 head0.006
GPT teacher head0.223
Teacher spread0.217 · 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

Citations1
Published2025
Admission routes1
Has abstractyes

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