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Record W2143208199 · doi:10.1051/0004-6361/201014672

<i>Herschel</i>-PACS spectroscopy of the intermediate mass protostar NGC 7129 FIRS 2

2010· article· en· W2143208199 on OpenAlexaff
M. Fich, Doug Johnstone, T. A. van Kempen, C. McCoey, A. Fuente, P. Caselli, L. E. Kristensen, R. Plume, J. Cernicharo, G. J. Herczeg, E. F. van Dishoeck, S. F. Wampfler, P. Gaufre, J. Gill, Hamid Javadi, M. Justen, W. M. Laauwen, W. Luinge, V. Ossenkopf, John C. Pearson, R. Bachiller, A. Baudry, M. Benedettini, E. A. Bergin, A. O. Benz, P. Bjerkeli, G. Blake, Sylvain Bontemps, J. Braine, S. Bruderer, C. Codella, F. Daniel, A. M. Di Giorgio, C. Dominik, S. D. Doty, P. Encrenaz, T. Giannini, J. R. Goicoechea, Th. de Graauw, F. Helmich, F. Herpin, M. R. Hogerheijde, T. Jacq, J. K. Jørgensen, Bengt Larsson, D. C. Lis, R. Liseau, M. Marseille, Gary J. Melnick, B. Nisini, M. Olberg, B. Parise, C. Risacher, J. Santiago, P. Saraceno, R. Shipman, M. Tafalla, F. van der Tak, R. Visser, F. Wyrowski, U. A. Yíldíz

Bibliographic record

VenueAstronomy and Astrophysics · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsWestern UniversityNational Research Council CanadaUniversity of CalgaryUniversity of VictoriaHerzberg Institute of AstrophysicsUniversity of Waterloo
FundersScience and Technology Facilities CouncilJet Propulsion LaboratoryStockholms UniversitetChalmers Tekniska HögskolaEidgenössische Technische Hochschule ZürichCalifornia Institute of TechnologyNational Aeronautics and Space Administration
KeywordsPhysicsEmission spectrumAstrophysicsEnvelope (radar)ProtostarSpectroscopyLine (geometry)Spectral lineExcitationPhotonStar formationAtomic physicsStarsAstronomyOptics

Abstract

fetched live from OpenAlex

Aims. We present preliminary results of the first Herschel spectroscopic observations of NGC 7129 FIRS2, an intermediate mass star-forming region. We attempt to interpret the observations in the framework of an in-falling spherical envelope.Methods. The PACS instrument was used in line spectroscopy mode (R = 1000–5000) with 15 spectral bands between 63 and 185 μm. This provided good detections of 26 spectral lines seen in emission, including lines of H2O, CO, OH, O I, and C II.Results. Most of the detected lines, particularly those of H2O and CO, are substantially stronger than predicted by the spherical envelope models, typically by several orders of magnitude. In this paper we focus on what can be learned from the detected CO emission lines.Conclusions. It is unlikely that the much stronger than expected line emission arises in the (spherical) envelope of the YSO. The region hot enough to produce such high excitation lines within such an envelope is too small to produce the amount of emission observed. Virtually all of this high excitation emission must arise in structures such as as along the walls of the outflow cavity with the emission produced by a combination of UV photon heating and/or non-dissociative shocks.

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 score0.010
Threshold uncertainty score0.020

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 communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.208
Teacher spread0.204 · 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

Citations30
Published2010
Admission routes1
Has abstractyes

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