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Record W4398782398 · doi:10.1093/mnras/stae1320

Multiple chemical tracers finally unveil the intricate NGC 1333 IRAS 4A outflow system. FAUST XVI

2024· article· en· W4398782398 on OpenAlexaff
Layal Chahine, C. Ceccarelli, M. De Simone, C. J. Chandler, C. Codella, L. Podio, A. López-Sepulcre, Nami Sakai, Laurent Loinard, Mathilde Bouvier, P. Caselli, C. Vastel, E. Bianchi, Nicolás Cuello, F. Fontani, Doug Johnstone, G. Sabatini, Tomoyuki Hanawa, Z. Zhang, Yuri Aikawa, G. Busquet, E. Caux, Aurore Durán, Eric Herbst, F. Ménard, Dominique Segura-Cox, Brian Svoboda, Nadia Balucani, Steven B. Charnley, F. Dulieu, Lucy Evans, D. Fedele, Siyi Feng, Tetsuya Hama, Tomoya Hirota, Andrea Isella, Izaskun Jiménez-Serra, B. Leflóch, Luke T Maud, María José Maureira, A. Miotello, G. Moellenbrock, Hideko Nomura, Yasuhiro Oba, Satoshi Ohashi, Yuki Okoda, Yoko Oya, J. E. Pineda, Albert Rimola, Takeshi Sakai, Yancy L. Shirley, L. Testi, S. Viti, Naoki Watanabe, Yoshimasa Watanabe, Yichen Zhang, S. Yamamoto

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of VictoriaHerzberg Institute of Astrophysics
FundersNational Science CouncilNational Astronomical Observatory of JapanEuropean CommissionHorizon 2020 Framework ProgrammeDeutsche ForschungsgemeinschaftH2020 European Research CouncilPlanetary Science DivisionNational Institutes of Natural SciencesNational Aeronautics and Space AdministrationNational Radio Astronomy ObservatoryNational Science Foundation
KeywordsPhysicsProtostarOutflowAstrophysicsRedshiftJet (fluid)AstronomyPrecessionStar formationStarsGalaxy

Abstract

fetched live from OpenAlex

ABSTRACT The exploration of outflows in protobinary systems presents a challenging yet crucial endeavour, offering valuable insights into the dynamic interplay between protostars and their evolution. In this study, we examine the morphology and dynamics of jets and outflows within the IRAS 4A protobinary system. This analysis is based on ALMA observations of SiO(5–4), H2CO(30, 3–20, 3), and HDCO(41, 4–31, 3) with a spatial resolution of ∼150 au. Leveraging an astrochemical approach involving the use of diverse tracers beyond traditional ones has enabled the identification of novel features and a comprehensive understanding of the broader outflow dynamics. Our analysis reveals the presence of two jets in the redshifted emission, emanating from IRAS 4A1 and IRAS 4A2, respectively. Furthermore, we identify four distinct outflows in the region for the first time, with each protostar, 4A1 and 4A2, contributing to two of them. We characterize the morphology and orientation of each outflow, challenging previous suggestions of bends in their trajectories. The outflow cavities of IRAS 4A1 exhibit extensions of 10 and 13 arcsec with position angles (PA) of 0° and -12°, respectively, while those of IRAS 4A2 are more extended, spanning 18 and 25 arcsec with PAs of 29° and 26°. We propose that the misalignment of the cavities is due to a jet precession in each protostar, a notion supported by the observation that the more extended cavities of the same source exhibit lower velocities, indicating they may stem from older ejection events.

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 score0.009
Threshold uncertainty score0.018

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 studies0.0000.000
Scholarly communication0.0010.000
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 head0.203
Teacher spread0.195 · 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

Citations10
Published2024
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicAstrophysics and Star Formation Studies→French-language works237,207→