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Record W2152644825 · doi:10.1051/0004-6361/201015109

CH<sup>+</sup>(1–0) and<sup>13</sup>CH<sup>+</sup>(1–0) absorption lines in the direction of massive star-forming regions

2010· article· en· W2152644825 on OpenAlexaff
É. Falgarone, B. Godard, J. Cernicharo, M. De Luca, Maryvonne Gérin, T. G. Phillips, J. H. Black, D. C. Lis, T. A. Bell, F. Boulanger, A. Coutens, E. Dartois, P. Encrenaz, Thomas F. Giesen, J. R. Goicoechea, P. F. Goldsmith, H. M. Sen Gupta, C. Gry, P. Hennebelle, Eric Herbst, P. Hily-Blant, C. Joblin, Marzena Kaźmierczak, Robert Kołos, J. Krełowski, J. Martín‐Pintado, Raquel Rodriguez Monje, B. Mookerjea, David A. Neufeld, M. Pérault, J. C. Pearson, Carina M. Persson, R. Plume, M. Salez, M. Schmidt, Paule Sonnentrucker, J. Stützki, D. Teyssier, C. Vastel, Shanshan Yu, K. M. Menten, T. R. Geballe, Stephan Śchlemmer, R. Shipman, A. G. G. M. Tielens, S. Philipp, A. Cros, J. Žmuidzinas, Lorene Samoska, K. Klein, A. Lorenzani, R. Szczerba, I. Péron, Ph. Caïs, P. Gaufre, A. Cros, Laurent Ravera, P. Morris, S. Lord, P. Planesas

Bibliographic record

VenueAstronomy and Astrophysics · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of WaterlooUniversity of Calgary
FundersEidgenössische Technische Hochschule ZürichCentre National d’Etudes SpatialesCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationStockholms UniversitetMinisterstwo Edukacji i NaukiChalmers Tekniska HögskolaNational Science Foundation
KeywordsPhysicsInterstellar mediumAnalytical Chemistry (journal)Carbon-12Atomic physicsNuclear reactionAstrophysicsChemistryGalaxy

Abstract

fetched live from OpenAlex

We report the detection of the ground-state rotational transition of the methylidyne cation CH+ and its isotopologue 13CH+ toward the remote massive star-forming regions W33A, W49N, and W51 with the HIFI instrument onboard the Herschel satellite. Both lines are seen only in absorption against the dust continuum emission of the star-forming regions. The CH+ absorption is saturated over almost the entire velocity ranges sampled by the lines-of-sight that include gas associated with the star-forming regions (SFR) and Galactic foreground material. The CH+ column densities are inferred from the optically thin components. A lower limit of the isotopic ratio [ 12CH+] /[ 13CH+] > 35.5 is derived from the absorptions of foreground material toward W49N. The column density ratio, N(CH+)/N(HCO+), is found to vary by at least a factor 10, between 4 and >40, in the Galactic foreground material. Line-of-sight 12CH+ average abundances relative to total hydrogen are estimated. Their average value, N(CH+)/NH > 2.6×10-8, is higher than that observed in the solar neighborhood and confirms the high abundances of CH+ in the Galactic interstellar medium. We compare this result to the predictions of turbulent dissipation regions (TDR) models and find that these high abundances can be reproduced for the inner Galaxy conditions. It is remarkable that the range of predicted N(CH+)/N(HCO+) ratios, from 1 to ~50, is comparable to that observed.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.010

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)0.0030.000

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 head0.009
GPT teacher head0.221
Teacher spread0.212 · 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

Citations70
Published2010
Admission routes1
Has abstractyes

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