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Record W4413489102 · doi:10.3847/1538-4365/adf203

An S-shaped Filament Formed Due to Cloud–Cloud Collision in Molecular Cloud G178.28-00.61

2025· article· en· W4413489102 on OpenAlexafffund
Tianwei Zhang, Tie Liu, Yuefang Wu, Linjing Feng, Sihan Jiao, D. Ward–Thompson, A. Traficante, H. J. Fraser, James Di Francesco, Doug Johnstone, P. F. Goldsmith, Yasuo Doi, Xunchuan Liu, Chang Won Lee, Fengwei Xu, Ram Kesh Yadav, G. J. White, L. Bronfman, Yi‐Jehng Kuan, Donghui Quan

Bibliographic record

VenueThe Astrophysical Journal Supplement Series · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of VictoriaHerzberg Institute of Astrophysics
FundersNatural Sciences and Engineering Research Council of CanadaUniversity of California, Los AngelesJet Propulsion LaboratoryNational Astronomical Observatory of JapanNational Aeronautics and Space AdministrationKorea Astronomy and Space Science InstituteChina Postdoctoral Science FoundationKey Research and Development Program of Zhejiang ProvinceChinese Academy of SciencesNational Key Research and Development Program of ChinaThailand Science Research and InnovationNational Astronomical Research Institute of ThailandNational Natural Science Foundation of ChinaAgencia Nacional de Investigación y DesarrolloCalifornia Institute of TechnologyAcademia Sinica
KeywordsCloud computingProtein filamentCollisionComputer scienceMaterials scienceComputer securityOperating systemComposite material

Abstract

fetched live from OpenAlex

Abstract We present compelling observational evidence supporting G178.28-00.61 as an early-stage candidate for cloud–cloud collision (CCC), with indications of the formation of an S-shaped filament, evenly separated dense cores, and young star clusters. The observations of CO molecular line emission demonstrate the existence of two interacting molecular clouds with systemic velocities of 0.8 km s−1 and −1.2 km s−1, respectively. The convergence zone of these two clouds reveals an S-shaped filament in the James Clerk Maxwell Telescope 850 μm continuum image, suggesting cloud interaction. In line with expectations from CCC simulations, broad bridging features are discernible in the position–velocity diagrams. An elevated concentration of identified Class I and II young stellar objects along the filament at the intersection area further supports the hypothesis of a collision-induced origin. This observation could be explained by a recent MHD model of CCC, which predicts a similar morphology, scale, density, and unbound status, as well as the orientation of the polarization.

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 score0.005
Threshold uncertainty score0.010

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
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 head0.007
GPT teacher head0.263
Teacher spread0.256 · 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

Citations0
Published2025
Admission routes2
Has abstractyes

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