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Record W4408883279 · doi:10.1051/0004-6361/202453386

FAUST

2025· article· en· W4408883279 on OpenAlexaff
Tomoya Hirota, B. Leflóch, Yoko Oya, Mathilde Bouvier, Steven B. Charnley, Izaskun Jiménez-Serra, A. López-Sepulcre, A. Miotello, J. Ospina-Zamudio, C. Vastel, S. Viti, C. J. Chandler, Brian Svoboda, C. Ceccarelli, C. Codella, Nami Sakai, Yuri Aikawa, Nadia Balucani, E. Bianchi, P. Caselli, E. Caux, Nicolás Cuello, M. De Simone, F. Dulieu, Lucy Evans, D. Fedele, Siyi Feng, F. Fontani, Tetsuya Hama, Tomoyuki Hanawa, Eric Herbst, Andrea Isella, Doug Johnstone, Hauyu Baobab Liu, Laurent Loinard, L. T. Maud, María José Maureira, F. Ménard, G. Moellenbrock, Hideko Nomura, Yasuhiro Oba, Satoshi Ohashi, Yuki Okoda, J. E. Pineda, L. Podio, Albert Rimola, G. Sabatini, Takeshi Sakai, Dominique Segura-Cox, Yancy L. Shirley, L. Testi, Naoki Watanabe, Yoshimasa Watanabe, Yichen Zhang, Satoshi Yamamoto

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of VictoriaHerzberg Institute of Astrophysics
FundersNational Institutes of Natural SciencesConsejo Nacional de Ciencia y TecnologíaHORIZON EUROPE Framework ProgrammeJapan Society for the Promotion of ScienceHorizon 2020 Framework ProgrammeDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoNational Science and Technology CouncilKorea Astronomy and Space Science InstituteNational Science FoundationNational Astronomical Observatory of JapanEuropean Regional Development FundEuropean CommissionMinistry of Education, Culture, Sports, Science and TechnologyAgencia Estatal de InvestigaciónNational Radio Astronomy Observatory
KeywordsPhysicsAstrophysicsFAUSTAstronomyLiterature

Abstract

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Context. While protostellar outflows are important in terms of mass accretion and angular momentum transport in star formation processes, high-resolution observations of outflows in protobinary systems are still sparse. Aims. We aim to reveal outflow structures traced by millimeter SiO emission in a low-mass protobinary system, L483. Methods. We observed the SiO (J = 5−4) line in L483 with the Atacama Large Millimeter/submillimeter Array (ALMA) as part of the large program FAUST (Fifty AU STudy of the chemistry in the disk/envelope systems of Solar-like protostars). The spatial and spectral resolutions were 0.39′′×0.30′′ (780 au×60 au) and 122 kHz (0.17 km s−1 at 217 GHz), respectively. The spectral lines of SO, CS, and C18O were also used to study the physical and dynamical properties of the SiO emitting regions. Results. Two SiO emission peaks are identified in the central part of L483, which have offsets of 100 au and 200 au toward the northeast (SiO-peak) and north (SiO-N), respectively, from the continuum peak. The SiO-peak shows only blueshifted emission with a broad linewidth of 5 km s−1, while that of SiO-N corresponds to the systemic velocity. Furthermore, weak and compact SiO emission components are distributed up to 2400 au away from the continuum position. They have narrow linewidths of ∼1 km s−1. One of these components is a blueshifted isolated emission feature, 2400 au northeast of the continuum peak, NE-cloud, located outside the east-west outflow lobes. The SiO abundances relative to H2 are 10−10−10−9 and 10−10 in the central part and more widely distributed components, respectively. These are intermediate values between those of strongly shocked regions caused by high-velocity outflows and quiescent molecular clouds. Conclusions. The central SiO emission could be interpreted as either two different outflows driven by both protostars or as an outflow ejected from one of the circumstellar disks in the binary system. The NE-cloud region is most likely explained as a remnant of an old shock produced by past outflow activity, as has been proposed for the low-mass protostar IRAS 15398–3359. The complex structures of the outflows traced by the SiO line could reflect dynamical processes of the newly formed protobinary system in L483.

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 categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Other · Consensus signal: Other
Teacher disagreement score0.458
Threshold uncertainty score0.000

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0020.002
Science and technology studies0.0020.001
Scholarly communication0.0050.002
Open science0.0020.003
Research integrity0.0020.001
Insufficient payload (model declined to judge)0.5420.416

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 head0.006
GPT teacher head0.221
Teacher spread0.215 · 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.

Study designNot applicable
Domainnot available
GenreOther

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

Citations1
Published2025
Admission routes1
Has abstractyes

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