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Record W3042366190 · doi:10.1093/mnrasl/slaa130

FAUST I. The hot corino at the heart of the prototypical Class I protostar L1551 IRS5

2020· article· en· W3042366190 on OpenAlexaff
E. Bianchi, C. J. Chandler, C. Ceccarelli, C. Codella, Nami Sakai, A. López-Sepulcre, L. T. Maud, G. Moellenbrock, Brian Svoboda, Yoshimasa Watanabe, Takeshi Sakai, F. Ménard, Yuri Aikawa, F. O. Alves, Nadia Balucani, Mathilde Bouvier, P. Caselli, E. Caux, S. B. Charnley, Spandan Choudhury, M. De Simone, F. Dulieu, Aurora Durán, Lucy Evans, Cécile Favre, D. Fedele, Siyi Feng, F. Fontani, Logan Francis, Tetsuya Hama, Tomoyuki Hanawa, Eric Herbst, Tomoya Hirota, Muneaki Imai, Andrea Isella, Izaskun Jiménez-Serra, Doug Johnstone, C. Kahane, B. Leflóch, Laurent Loinard, María José Maureira, S. Mercimek, A. Miotello, Shoji Mori, Riouhei Nakatani, Hideko Nomura, Yasuhiro Oba, Satoshi Ohashi, Yuki Okoda, J. Ospina-Zamudio, Yoko Oya, J. E. Pineda, L. Podio, Albert Rimola, Yancy L. Shirley, V. Taquet, L. Testi, C. Vastel, S. Viti, Naoki Watanabe, A. Witzel, Ci Xue, Yichen Zhang, Bo Zhao, Satoshi Yamamoto

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society Letters · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of VictoriaHerzberg Institute of Astrophysics
FundersH2020 European Research CouncilNational Institutes of Natural SciencesDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoFederación Española de Enfermedades RarasNational Astronomical Observatory of JapanEuropean CommissionAssociated UniversitiesJapan Society for the Promotion of ScienceConsejo Nacional de Ciencia y TecnologíaAgence Nationale de la RechercheNational Radio Astronomy ObservatoryKorea Astronomy and Space Science InstituteNational Science Foundation
KeywordsProtostarIsotopologueAstrophysicsPhysicsMethyl formateSubmillimeter ArrayAstrobiologyStar formationAstronomyMethanolChemistryStarsOrganic chemistry

Abstract

fetched live from OpenAlex

ABSTRACT The study of hot corinos in solar-like protostars has been so far mostly limited to the Class 0 phase, hampering our understanding of their origin and evolution. In addition, recent evidence suggests that planet formation starts already during Class I phase, which therefore represents a crucial step in the future planetary system chemical composition. Hence, the study of hot corinos in Class I protostars has become of paramount importance. Here, we report the discovery of a hot corino towards the prototypical Class I protostar L1551 IRS5, obtained within the ALMA (Atacama Large Millimeter/submillimeter Array) Large Program FAUST (Fifty AU STudy of the chemistry in the disc/envelope system of solar-like protostars). We detected several lines from methanol and its isotopologues (13CH3OH and CH2DOH), methyl formate, and ethanol. Lines are bright towards the north component of the IRS5 binary system, and a possible second hot corino may be associated with the south component. The methanol lines' non-LTE analysis constrains the gas temperature (∼100 K), density (≥1.5 × 108 cm−3), and emitting size (∼10 au in radius). All CH3OH and 13CH3OH lines are optically thick, preventing a reliable measure of the deuteration. The methyl formate and ethanol relative abundances are compatible with those measured in Class 0 hot corinos. Thus, based on this work, little chemical evolution from Class 0 to I hot corinos occurs.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.401
Threshold uncertainty score0.472

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0000.000
Science and technology studies0.0010.001
Scholarly communication0.0000.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.011
GPT teacher head0.205
Teacher spread0.194 · 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 teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
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

Citations49
Published2020
Admission routes1
Has abstractyes

Explore more

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