MétaCan
Menu
Back to cohort
Record W4391670836 · doi:10.1051/0004-6361/202348889

JWST Observations of Young protoStars (JOYS)

2024· preprint· en· W4391670836 on OpenAlexfundno aff
Łukasz Tychoniec, M. L. van Gelder, E. F. van Dishoeck, Logan Francis, W. R. M. Rocha, A. Caratti o Garatti, H. Beuther, C. Gieser, K. Justtanont, H. Linnartz, Valentin J. M. Le Gouellec, Giulia Perotti, R. Devaraj, Benoît Tabone, T. P. Ray, Nashanty G. C. Brunken, Y. Chen, Patrick Kavanagh, Pamela Klaassen, K. Slavicinska, M. Güdel, Göran Östlin

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsnot available
FundersEuropean Research CouncilNederlandse Onderzoekschool Voor AstronomieMax-Planck-GesellschaftDeutsches Zentrum für Luft- und RaumfahrtCentre National d’Etudes SpatialesIrish Research CouncilSwedish National Space AgencyNational Radio Astronomy ObservatoryNational Institutes of Natural SciencesEnterprise IrelandNational Astronomical Observatory of JapanNational Aeronautics and Space AdministrationDanmarks GrundforskningsfondScience Foundation IrelandBelgian Federal Science Policy OfficeNational Science FoundationEuropean Space AgencySpace Telescope Science InstituteKorea Astronomy and Space Science InstituteDeutsche ForschungsgemeinschaftScience and Technology Facilities CouncilUK Space AgencyNational Research FoundationNederlandse Organisatie voor Wetenschappelijk OnderzoekCanadian Space Agency
KeywordsProtostarAccretion (finance)Class (philosophy)Accretion discPhysicsAstrophysicsAstronomyGeologyComputer scienceStarsStar formationArtificial intelligence

Abstract

fetched live from OpenAlex

Context. Accretion and ejection dictate the outcomes of star and planet formation processes. The mid-infrared (MIR) wavelength range offers key tracers of processes that have been difficult to detect and spatially resolve in protostars until now. Aims. We aim to characterize the interplay between accretion and ejection in the low-mass Class I protobinary system TMC1, comprising two young stellar objects: TMC1-W and TMC1-E at a 85 au separation. Methods. Using the James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) observations in 5–28 μm range, we measured the intensities of emission lines of H 2 , atoms, and ions, for instance, the [Fe II] and [Ne II], and HI recombination lines. We analyzed the spatial distribution of the different species using the MIRI Medium Resolution Spectrometer (MRS) capabilities to spatially resolve emission at 0″​​.2–0″​​.7 scales. we compared these results with the corresponding Atacama Large Millimeter/submillimeter Array (ALMA) maps tracing cold gas and dust. Results. We detected H 2 outflow coming from TMC1-E, with no significant H 2 emission from TMC1-W. The H 2 emission from TMC1-E outflow appears narrow and extends to wider opening angles with decreasing E up from S(8) to S(1) rotational transitions, indicating the disk wind as its origin. The outflow from TMC1-E protostar shows spatially extended emission lines of [Ne II], [Ne III], [Ar II], and [Ar III], with their line ratios consistent with UV radiation as a source of ionization. With ALMA, we detected an accretion streamer infalling from > 1000 au scales onto the TMC1-E component. The TMC1-W protostar powers a collimated jet, detected with [Fe II] and [Ni II], making it consistent with energetic flow. A much weaker ionized jet is observed from TMC1-E, and both jets appear strikingly parallel to each other, indicating that the disks are co-planar. TMC1-W is associated with strong emission from hydrogen recombination lines, tracing the accretion onto the young star. Conclusions. MIRI-MRS observations provide an unprecedented view of protostellar accretion and ejection processes on 20 au scales. Observations of a binary Class I protostellar system show that the two processes are clearly intertwined, with accretion from the envelope onto the disk influencing a wide-angle wind ejected on disk scales. Finally, the accretion from the protostellar disk onto the protostar is associated with the source launching a collimated high-velocity jet within the innermost regions of the disk.

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 categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: Theoretical or conceptual
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.353
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.001
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 head0.020
GPT teacher head0.236
Teacher spread0.216 · 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.

Study designTheoretical or conceptual
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

Citations31
Published2024
Admission routes1
Has abstractyes

Explore more

Same venueAstronomy and AstrophysicsSame topicAstrophysical Phenomena and ObservationsFrench-language works237,207