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Record W4411715721 · doi:10.1093/mnras/staf1002

FAUST – XXVII. The circumbinary disc and the outflow of the L 1551 IRS 5 binary system

2025· article· en· W4411715721 on OpenAlexaff
Aurora Durán, Laurent Loinard, P. R. Rivera-Ortíz, Geovanni Cortés-Rangel, E. Bianchi, P. Caselli, C. Ceccarelli, C. J. Chandler, C. Codella, Nicolás Cuello, M. De Simone, Tomoyuki Hanawa, Doug Johnstone, F. Ménard, María José Maureira, A. Miotello, L. Podio, Takeshi Sakai, G. Sabatini, L. Testi, C. Vastel, Ziwei Zhang, Nami Sakai, Satoshi Yamamoto

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of VictoriaHerzberg Institute of Astrophysics
FundersNational Institutes of Natural SciencesDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoHORIZON EUROPE Framework ProgrammeKorea Astronomy and Space Science InstituteNational Science FoundationConsejo Nacional de Ciencia y TecnologíaNational Science CouncilNational Astronomical Observatory of JapanEuropean CommissionNational Radio Astronomy Observatory
KeywordsPhysicsCircumbinary planetAstrophysicsAstronomyOutflowBinary numberBinary starBinary systemStars

Abstract

fetched live from OpenAlex

ABSTRACT Using continuum and $\mbox{C}^{18}\mbox{O}\:(2-1)$ line data obtained from the large ALMA (Atacama Large Millimeter/submillimeter Array) programme FAUST (Fifty AU STudy of the chemistry in the disc/envelope system of solar-like protostars), we studied the structure of the protostellar binary system L 1551 IRS 5 at scales between 30 and 3000 au to constrain its properties, from the circumstellar and circumbinary discs up to the envelope and outflow scales, which exhibits complex and entangled structures at the scales of its inner and outer envelopes, presumably caused by the influence of the central binary. Assuming a dust-to-gas ratio of 100, we calculated the dust + gas mass for the circumbinary disc and each circumstellar disc of the binary, obtaining 0.018 M$_\odot$ for the circumbinary disc, 0.004 and 0.002 M$_\odot$ for the northern and southern circumstellar disc, respectively. From the line emission, we retrieved the gas masses for each structure component. With the $\mbox{C}^{18}\mbox{O}\:(2-1)$ position–velocity diagram along the circumbinary disc, we were able to constrain the centrifugal barrier, ${r_{CB}=55}$ au, update the specific angular momentum, ${j\sim 270}$ au km s$^{-1}$. We built an analytical model that can be used to predict the influence of the morphology of the outflow and a few dynamic features that can reproduce the system emission, allowing us to explain and discern the outflow contribution from the complex emission due to the binary. Additionally, we inferred the density power-law index, ${\alpha =1.7}$, and the envelope rotation velocity, $\upsilon _{c}=2$ km s$^{-1}$. Finally, the observations gave us the physical constraints to obtain a coherent outflow model for L 1551 IRS 5.

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 score0.021
Threshold uncertainty score0.043

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 studies0.0000.000
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 head0.004
GPT teacher head0.193
Teacher spread0.189 · 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

Citations2
Published2025
Admission routes1
Has abstractyes

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