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Record W2154230204 · doi:10.1051/0004-6361/201014609

Physical properties of the Sh2-104 H II region as seen by<i>Herschel</i>

2010· article· en· W2154230204 on OpenAlexaff
J. A. Rodón, A. Zavagno, J.‐P. Baluteau, L. D. Anderson, E. T. Polehampton, A. Abergel, F. Motte, Sylvain Bontemps, P. A. R. Ade, Paulo André, H. Arab, C. Beichman, J.-P. Bernard, K. Blagrave, F. Boulanger, Martin Cohen, M. Compiègne, P. Cox, E. Dartois, G. R. Davis, R. J. Emery, T. Fulton, C. Gry, E. Habart, M. Halpern, M. Huang, C. Joblin, Scott C. Jones, J. M. Kirk, G. Lagache, T. T. Y. Lin, S. C. Madden, G. Makiwa, P. G. Martin, M.-A. Miville-Deschênes, S. Molinari, H. Moseley, D. A. Naylor, K. Okumura, François Orieux, D. Pinheiro Gonçalves, Thomas Rodet, D. Russeil, P. Saraceno, S. Sidher, Locke D. Spencer, B. M. Swinyard, D. Ward–Thompson, G. J. White

Bibliographic record

VenueAstronomy and Astrophysics · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of British ColumbiaCanadian Institute for Theoretical AstrophysicsUniversity of Lethbridge
FundersNational Astronomical Observatories, Chinese Academy of SciencesCentro de Instrumentación Científico-Técnica, Universidad de JaénMax-Planck-Institut für AstronomieScience and Technology Facilities CouncilBundesministerium für Verkehr, Innovation und TechnologieCentre National de la Recherche ScientifiqueNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyAgence Nationale de la RechercheImperial College LondonCentre National d’Etudes Spatiales
KeywordsPhysicsIsotopologueAstrophysicsStarsPhotometry (optics)Spectral indexInfraredSpectral lineSpectral energy distributionEmissivityAstronomyGalaxyOptics

Abstract

fetched live from OpenAlex

Context. Sh2-104 is a Galactic H ii region with a bubble morphology, detected at optical and radio wavelengths. It is considered the first observational confirmation of the collect-and-collapse model of triggered star-formation. Aims. We aim to analyze the dust and gas properties of the Sh2-104 region to better constrain its effect on local future generations of stars. In addition, we investigate the relationship between the dust emissivity index β and the dust temperature, Tdust.Methods. Using Herschel PACS and SPIRE images at 100, 160, 250, 350 and 500 μm we determine Tdust and β throughout Sh2-104, fitting the spectral energy distributions (SEDs) obtained from aperture photometry. With the SPIRE Fourier-transform spectrometer (FTS) we obtained spectra at different positions in the Sh2-104 region. We detect J-ladders of 12CO and 13CO, with which we derive the gas temperature and column density. We also detect proxies of ionizing flux as the [Nii] 3P1-3P0 and [Ci] 3P2–3P1 transitions.Results. We find an average value of β ~ 1.5 throughout Sh2-104, as well as a Tdust difference between the photodissociation region (PDR, ~25 K) and the interior (~40 K) of the bubble. We recover the anti-correlation between β and dust temperature reported numerous times in the literature. The relative isotopologue abundances of CO appear to be enhanced above the standard ISM values, but the obtained value is very preliminary and is still affected by large uncertainties.

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 score0.009
Threshold uncertainty score0.019

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
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 head0.007
GPT teacher head0.196
Teacher spread0.189 · 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

Citations25
Published2010
Admission routes1
Has abstractyes

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