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Record W2137793512 · doi:10.1051/0004-6361/201015107

<i>Herschel</i>observations of EXtra-Ordinary Sources (HEXOS): detecting spiral arm clouds by CH absorption lines

2010· article· en· W2137793512 on OpenAlexaff
Sheng‐Li Qin, P. Schilke, C. Comito, T. Möller, R. Rolffs, H. S. P. Müller, А. Беллоче, K. M. Menten, D. C. Lis, T. G. Phillips, E. A. Bergin, T. A. Bell, N. R. Crockett, G. A. Blake, S. Cabrit, E. Caux, C. Ceccarelli, J. Cernicharo, F. Daniel, Marie-Lise Dubernet, M. Emprechtinger, P. Encrenaz, É. Falgarone, Maryvonne Gérin, Thomas F. Giesen, J. R. Goicoechea, P. F. Goldsmith, H. M. Sen Gupta, Eric Herbst, C. Joblin, Doug Johnstone, W. D. Langer, S. D. Lord, S. Maret, P. G. Martin, Gary J. Melnick, P. Morris, J. A. Murphy, David A. Neufeld, V. Ossenkopf, L. Pagani, John C. Pearson, M. Pérault, R. Plume, M. Salez, Stephan Śchlemmer, J. Stützki, N. Trappe, F. F. S. van der Tak, C. Vastel, S. Wang, H. W. Yorke, Shanshan Yu, J. Žmuidzinas, A. C. A. Boogert, R. Güsten, P. Hartogh, N. Honingh, A. Karpov, J. Kooi, Jean-Michel Krieg, R. Schieder, M. C. Díez-González, R. Bachiller, J. Martín‐Pintado, W. Baechtold, M. Olberg, L. Nordh, J. Gill, Goutam Chattopadhyay

Bibliographic record

VenueAstronomy and Astrophysics · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of CalgaryCanadian Institute for Theoretical AstrophysicsNational Research Council CanadaUniversity of TorontoHerzberg Institute of Astrophysics
FundersStockholms UniversitetChalmers Tekniska HögskolaEidgenössische Technische Hochschule ZürichCalifornia Institute of Technology
KeywordsSpiral galaxyExtinction (optical mineralogy)PhysicsAstrophysicsLine-of-sightGalaxyAbsorption (acoustics)Molecular cloudEnvelope (radar)Spectral lineLine (geometry)Absorption spectroscopyOpticsGeometryAstronomyStars

Abstract

fetched live from OpenAlex

We have observed CH absorption lines (J = 3/2, N = 1 J = 1/2, N = 1) against the continuum source Sgr B2(M) using the Herschel/HIFI instrument. With the high spectral resolution and wide velocity coverage provided by HIFI, 31 CH absorption features with different radial velocities and line widths are detected and identified. The narrower line width and lower column density clouds show “spiral arm” cloud characteristics, while the absorption component with the broadest line width and highest column density corresponds to the gas from the Sgr B2 envelope. The observations show that each “spiral arm” harbors multiple velocity components, indicating that the clouds are not uniform and that they have internal structure. This line-of-sight through almost the entire Galaxy offers unique possibilities to study the basic chemistry of simple molecules in diffuse clouds, as a variety of different cloud classes are sampled simultaneously. We find that the linear relationship between CH and H2 column densities found at lower AV by UV observations does not continue into the range of higher visual extinction. There, the curve flattens, which probably means that CH is depleted in the denser cores of these clouds.

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 score0.005
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)0.0010.000

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 head0.013
GPT teacher head0.225
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

Citations37
Published2010
Admission routes1
Has abstractyes

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