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Record W2153813522 · doi:10.1051/0004-6361/201015106

Reversal of infall in SgrB2(M) revealed by<i>Herschel</i>/HIFI observations of HCN lines at THz frequencies

2010· article· en· W2153813522 on OpenAlexaff
R. Rolffs, P. Schilke, C. Comito, E. A. Bergin, F. F. S. van der Tak, D. C. Lis, Sheng‐Li Qin, K. M. Menten, R. Güsten, T. A. Bell, G. A. Blake, E. Caux, C. Ceccarelli, J. Cernicharo, N. R. Crockett, F. Daniel, Marie-Lise Dubernet, M. Emprechtinger, P. Encrenaz, Maryvonne Gérin, Thomas F. Giesen, J. R. Goicoechea, P. F. Goldsmith, H. M. Sen Gupta, Eric Herbst, C. Joblin, Doug Johnstone, W. D. Langer, W. D. Latter, S. D. Lord, S. Maret, P. G. Martin, Gary J. Melnick, P. Morris, H. S. P. Müller, J. A. Murphy, V. Ossenkopf, J. C. Pearson, M. Pérault, T. G. Phillips, R. Plume, Stephan Śchlemmer, J. Stützki, N. Trappe, C. Vastel, S. Wang, H. W. Yorke, Shanshan Yu, J. Žmuidzinas, 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
FundersEidgenössische Technische Hochschule ZürichCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationStockholms UniversitetChalmers Tekniska HögskolaNational Science Foundation
KeywordsPhysicsIsotopologueAstrophysicsLine (geometry)Radiative transferOpacityAccretion (finance)Molecular cloudStar formationAstronomySpectral lineGalaxyGeometryStarsOptics

Abstract

fetched live from OpenAlex

Aims. To investigate the accretion and feedback processes in massive star formation, we analyze the shapes of emission lines from hot molecular cores, whose asymmetries trace infall and expansion motions.Methods. The high-mass star forming region SgrB2(M) was observed with Herschel/HIFI (HEXOS key project) in various lines of HCN and its isotopologues, complemented by APEX data. The observations are compared to spherically symmetric, centrally heated models with density power-law gradient and different velocity fields (infall or infall+expansion), using the radiative transfer code RATRAN. Results. The HCN line profiles are asymmetric, with the emission peak shifting from blue to red with increasing J and decreasing line opacity (HCN to H13CN). This is most evident in the HCN 12–11 line at 1062 GHz. These line shapes are reproduced by a model whose velocity field changes from infall in the outer part to expansion in the inner part.Conclusions. The qualitative reproduction of the HCN lines suggests that infall dominates in the colder, outer regions, but expansion dominates in the warmer, inner regions. We are thus witnessing the onset of feedback in massive star formation, starting to reverse the infall and finally disrupting the whole molecular cloud. To obtain our result, the THz lines uniquely covered by HIFI were critically important.

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 score0.004
Threshold uncertainty score0.008

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 head0.012
GPT teacher head0.217
Teacher spread0.205 · 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

Citations29
Published2010
Admission routes1
Has abstractyes

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