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Record W4384699418 · doi:10.3847/2041-8213/acdddf

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Forming Quadruple System with Continuum “Ribbons” and Intricate Outflows

2023· article· en· W4384699418 on OpenAlexafffund
Qiuyi Luo, Tie Liu, A. T. Lee, Stella S. R. Offner, James Di Francesco, Doug Johnstone, M. Juvela, P. F. Goldsmith, Sheng‐Li Qin, Xiaofeng Mai, Xunchuan Liu, Patricio Sanhueza, Fengwei Xu, Ken’ichi Tatematsu, Somnath Dutta, Huei-Ru Vivien Chen, Shanghuo Li, A. Y. Yang, Sheng‐Yuan Liu, Chin‐Fei Lee, Naomi Hirano, Chang Won Lee, Dipen Sahu, Hsien Shang, Shih‐Ying Hsu, L. Bronfman, Woojin Kwon, Mark G. Rawlings, David Eden, Xing Lu, Qilao Gu, Zhiyuan Ren, D. Ward–Thompson, Zhi-Qiang Shen

Bibliographic record

VenueThe Astrophysical Journal Letters · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of VictoriaHerzberg Institute of Astrophysics
FundersNational Key Research and Development Program of China Stem Cell and Translational ResearchNational Institutes of Natural SciencesJet Propulsion LaboratoryNatural Sciences and Engineering Research Council of CanadaNational Science and Technology CouncilMinistry of Science and ICT, South KoreaNational Astronomical Observatory of JapanAgencia Nacional de Investigación y DesarrolloNational Research Foundation of KoreaMassachusetts Green High Performance Computing CenterChinese Academy of SciencesScience and Technology Facilities CouncilNational Research FoundationKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyScience and Engineering Research BoardJapan Society for the Promotion of ScienceAcademy of FinlandNational Natural Science Foundation of ChinaNational Radio Astronomy ObservatoryNational Science Foundation
KeywordsPhysicsAstrophysicsSubmillimeter ArrayProtostarMillimeterMolecular cloudOutflowStar formationYoung stellar objectAstronomyStars

Abstract

fetched live from OpenAlex

Abstract One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations toward a forming quadruple protostellar system, G206.93-16.61E2, in the Orion B molecular cloud. ALMA 1.3 mm continuum emission reveals four compact objects, of which two are Class I young stellar objects and the other two are likely in prestellar phase. The 1.3 mm continuum emission also shows three asymmetric ribbon-like structures that are connected to the four objects, with lengths ranging from ∼500 to ∼2200 au. By comparing our data with magnetohydrodynamic simulations, we suggest that these ribbons trace accretion flows and also function as gas bridges connecting the member protostars. Additionally, ALMA CO J = 2−1 line emission reveals a complicated molecular outflow associated with G206.93-16.61E2, with arc-like structures suggestive of an outflow cavity viewed pole-on.

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 score0.007
Threshold uncertainty score0.014

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
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 head0.013
GPT teacher head0.224
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

Citations3
Published2023
Admission routes2
Has abstractyes

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