MétaCan
Menu
Back to cohort
Record W4295732806 · doi:10.1093/mnras/stac2559

PHANGS: constraining star formation time-scales using the spatial correlations of star clusters and giant molecular clouds

2022· article· en· W4295732806 on OpenAlexaff
J. Turner, Daniel A. Dale, James Lilly, M. Boquien, Sinan Deger, Janice Lee, Bradley C. Whitmore, Gagandeep S. Anand, Samantha M. Benincasa, Frank Bigiel, Guillermo A. Blanc, Mélanie Chevance, Éric Emsellem, Christopher M. Faesi, Simon C. O. Glover, Kathryn Grasha, Annie Hughes, Ralf S. Klessen, Kathryn Kreckel, J. M. Diederik Kruijssen, Adam K. Leroy, Hsi-An Pan, Erik Rosolowsky, Andreas Schruba, Thomas G. Williams

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of Alberta
FundersH2020 European Research CouncilNational Institutes of Natural SciencesAustralian Research CouncilFondo Nacional de Desarrollo Científico y TecnológicoNational Astronomical Observatory of JapanJet Propulsion LaboratoryMinistry of Science and Technology, TaiwanEuropean School of OncologyCalifornia Institute of TechnologyEuropean CommissionMinistry of Science and TechnologyNational Science FoundationU.S. Nuclear Regulatory CommissionAeroDynamic SolutionsDeutsche ForschungsgemeinschaftSpace Telescope Science InstituteKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationEntomological Society of America
KeywordsPhysicsAstrophysicsStar formationStar clusterMolecular cloudSpiral galaxyAstronomyIntergalactic starStar (game theory)StarsCluster (spacecraft)Lenticular galaxy

Abstract

fetched live from OpenAlex

ABSTRACT In the hierarchical view of star formation, giant molecular clouds (GMCs) undergo fragmentation to form small-scale structures made up of stars and star clusters. Here we study the connection between young star clusters and cold gas across a range of extragalactic environments by combining the high resolution (1″) PHANGS–ALMA catalogue of GMCs with the star cluster catalogues from PHANGS–HST. The star clusters are spatially matched with the GMCs across a sample of 11 nearby star-forming galaxies with a range of galactic environments (centres, bars, spiral arms, etc.). We find that after 4 − 6 Myr the star clusters are no longer associated with any gas clouds. Additionally, we measure the autocorrelation of the star clusters and GMCs as well as their cross-correlation to quantify the fractal nature of hierarchical star formation. Young (≤10 Myr) star clusters are more strongly autocorrelated on kpc and smaller spatial scales than the $\gt \, 10$ Myr stellar populations, indicating that the hierarchical structure dissolves over time.

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)0.002
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 score0.012
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
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 head0.009
GPT teacher head0.210
Teacher spread0.201 · 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 routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicAstrophysics and Star Formation StudiesFrench-language works237,207