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Record W2104529841 · doi:10.1051/0004-6361/201014577

Detection of interstellar oxidaniumyl: Abundant H<sub>2</sub>O<sup>+</sup>towards the star-forming regions DR21, Sgr B2, and NGC6334

2010· article· en· W2104529841 on OpenAlexaff
V. Ossenkopf, H. S. P. Müller, D. C. Lis, P. Schilke, Thomas A. Bell, S. Bruderer, E. A. Bergin, C. Ceccarelli, C. Comito, J. Stützki, A. Bacman, A. Baudry, A. O. Benz, M. Benedettini, Olivier Berné, G. Blake, A. C. A. Boogert, S. Bottinelli, F. Boulanger, S. Cabrit, P. Caselli, E. Caux, J. Cernicharo, C. Codella, A. Coutens, N. Crimier, N. R. Crockett, F. Daniel, Karine Demyk, P. Dieleman, C. Dominik, Marie-Lise Dubernet, M. Emprechtinger, P. Encrenaz, É. Falgarone, Kevin France, A. Fuente, Maryvonne Gérin, Thomas F. Giesen, A. M. Di Giorgio, J. R. Goicoechea, P. F. Goldsmith, R. Güsten, A. I. Harris, F. Helmich, Eric Herbst, P. Hily-Blant, K. Jacobs, T. Jacq, C. Joblin, Doug Johnstone, C. Kahane, Mihkel Kama, Thomas Klein, A. Klotz, C. Krämer, W. D. Langer, B. Leflóch, Christian Leinz, A. Lorenzani, S. D. Lord, S. Maret, P. G. Martin, J. Martín‐Pintado, C. McCoey, M. Melchior, Gary J. Melnick, K. M. Menten, B. Mookerjea, P. Morris, J. A. Murphy, David A. Neufeld, B. Nisini, S. Pacheco, L. Pagani, B. Parise, John C. Pearson, M. Pérault, T. G. Phillips, R. Plume, S.-L. Quin, Ricardo Rizzo, M. Röllig, M. Salez, P. Saraceno, Stephan Śchlemmer, R. Simon, K. Schüster, F. F. S. van der Tak, A. G. G. M. Tielens, D. Teyssier, N. Trappe, C. Vastel, S. Viti, Valentine Wakelam, Adam Walters, S. Wang, N. Whyborn, M. H. D. van der Wiel, H. W. Yorke, Shanshan Yu, J. Žmuidzinas

Bibliographic record

VenueAstronomy and Astrophysics · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of CalgaryWestern UniversityUniversity of WaterlooHerzberg Institute of AstrophysicsUniversity of Toronto
FundersScience and Technology Facilities CouncilEidgenössische Technische Hochschule ZürichStockholms UniversitetChalmers Tekniska HögskolaBundesministerium für Bildung und ForschungNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyJet Propulsion LaboratoryDeutsche ForschungsgemeinschaftNational Science Foundation
KeywordsPhysicsAstrophysicsSpectral lineHyperfine structureInterstellar mediumAbsorption spectroscopyAbsorption (acoustics)Line (geometry)Atomic physicsGalaxyAstronomyOptics

Abstract

fetched live from OpenAlex

Aims. We identify a prominent absorption feature at 1115 GHz, detected in first HIFI spectra towards high-mass star-forming regions, and interpret its astrophysical origin. Methods. The characteristic hyperfine pattern of the H2O+ ground-state rotational transition, and the lack of other known low-energy transitions in this frequency range, identifies the feature as H2O+ absorption against the dust continuum background and allows us to derive the velocity profile of the absorbing gas. By comparing this velocity profile with velocity profiles of other tracers in the DR21 star-forming region, we constrain the frequency of the transition and the conditions for its formation. Results. In DR21, the velocity distribution of H2O+ matches that of the [C ii] line at 158 μm and of OH cm-wave absorption, both stemming from the hot and dense clump surfaces facing the H ii-region and dynamically affected by the blister outflow. Diffuse foreground gas dominates the absorption towards Sgr B2. The integrated intensity of the absorption line allows us to derive lower limits to the H2O+ column density of 7.2 × 1012 cm-2 in NGC 6334, 2.3 × 1013 cm-2 in DR21, and 1.1 × 1015 cm-2 in Sgr B2.

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 score0.002
Threshold uncertainty score0.007

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)0.0020.000

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 head0.008
GPT teacher head0.199
Teacher spread0.191 · 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

Citations86
Published2010
Admission routes1
Has abstractyes

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