MétaCan
Menu
Back to cohort
Record W4405518896 · doi:10.1093/mnras/stae2773

Spiral arm, rotating structure, and outflow cavity in massive star-forming region G23.43−0.18

2024· article· en· W4405518896 on OpenAlexfundno aff
James O. Chibueze, C J Ugwu, Tomoya Hirota, Kee‐Tae Kim, Tie Liu, J.M. Vorster, Ji‐hyun Kang, Jungha Kim, Ross A. Burns, А. М. Соболев, Jihye Hwang, Chang‐Won Lee, Mi Kyoung Kim, Koichiro Sugiyama

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldBiochemistry, Genetics and Molecular Biology
TopicGeomagnetism and Paleomagnetism Studies
Canadian institutionsnot available
FundersNational Institutes of Natural SciencesUniversity of South AfricaMinistero degli Affari Esteri e della Cooperazione InternazionaleNational Astronomical Observatory of JapanNational Research Foundation of KoreaAlberta Livestock and Meat AgencyJapan Society for the Promotion of ScienceAcademy of FinlandNational Radio Astronomy ObservatoryDepartment of Science and Technology, Ministry of Science and Technology, IndiaNational Research Council CanadaNational Research FoundationMinistry of Education, Culture, Sports, Science and TechnologyMinistry of Education, Science and TechnologyKorea Astronomy and Space Science InstituteNational Science Foundation
KeywordsPhysicsOutflowSpiral (railway)Star (game theory)AstrophysicsAstronomySpiral galaxyStars

Abstract

fetched live from OpenAlex

ABSTRACT We confirmed the existence of a massive protocluster in G23.43−0.18 from our Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum and molecular line observations. We resolved the region into one main massive protostellar object, G23.43−0.18 A, one intermediate mass protostellar object, G23.43−0.18 B, and three low mass objects, G23.43−0.18 C1, G23.43–0.18 C2, and G23.43−0.18 C3. A spiral arm structure is observed in G23.43−0.18 B. G23.43−0.18 A 1.3 mm dust continuum emission showed a ‘butterfly’ morphology with clear evidence of the existence of a cavity and bipolar outflow with an inclination angle of 50$^\circ$. G23.43−0.18 B presents a compact rotating structure, and possibly an inner Keplerian disc, traced with methanol lines and powers a jet revealed by multiple compact emission peaks in CO, indicating episodic ejections every 300 yr. The presence of 6.7 GHz methanol masers in G23.43−0.18 A and G23.43−0.18 B are strong indications that both objects host massive protostars and are good sites to test some theories of the early evolutionary phases of massive stars.

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
Bibliometrics0.0010.001
Science and technology studies0.0010.000
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 head0.008
GPT teacher head0.214
Teacher spread0.206 · 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

Citations4
Published2024
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicGeomagnetism and Paleomagnetism StudiesFrench-language works237,207