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Record W2002064252 · doi:10.1051/0004-6361/201014603

Water cooling of shocks in protostellar outflows

2010· article· en· W2002064252 on OpenAlexaff
B. Nisini, M. Benedettini, C. Codella, T. Giannini, R. Liseau, David A. Neufeld, M. Tafalla, E. F. van Dishoeck, R. Bachiller, A. Baudry, A. O. Benz, E. A. Bergin, P. Bjerkeli, G. Blake, S. Bontemps, J. Braine, S. Bruderer, P. Caselli, J. Cernicharo, F. Daniel, P. Encrenaz, A. M. Di Giorgio, C. Dominik, S. D. Doty, M. Fich, A. Fuente, J. R. Goicoechea, Th. de Graauw, F. Helmich, G. J. Herczeg, F. Herpin, M. Hogerheijde, T. Jacq, Doug Johnstone, J. K. Jørgensen, Michael J. Kaufman, L. E. Kristensen, B. Larsson, D. C. Lis, M. Marseille, C. McCoey, Gary J. Melnick, M. Olberg, B. Parise, J. Pearson, R. Plume, C. Risacher, J. Santiago, P. Saraceno, R. F. Shipman, T. A. van Kempen, R. Visser, S. Viti, S. F. Wampfler, Friedrich Wyrowski, F. van der Tak, U. A. Yíldíz, B. Delforge, J.-P. Desbat, W. A. Hatch, I. Péron, R. Schieder, J. A. Stern, D. Teyssier, N. Whyborn

Bibliographic record

VenueAstronomy and Astrophysics · 2010
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsNational Research Council CanadaUniversity of CalgaryUniversity of VictoriaHerzberg Institute of AstrophysicsUniversity of Waterloo
FundersScience and Technology Facilities Council
KeywordsOutflowAstrophysicsPhysicsExcited stateStarsShock (circulatory)Line (geometry)Abundance (ecology)Intensity (physics)Emission spectrumAstronomyAtomic physicsSpectral lineMeteorologyOptics

Abstract

fetched live from OpenAlex

<i>Context. <i/>The far-IR/sub-mm spectral mapping facility provided by the <i>Herschel<i/>-PACS and HIFI instruments has made it possible to obtain, for the first time, images of H<sub>2<sub/>O emission with a spatial resolution comparable to ground based mm/sub-mm observations.<i>Aims. <i/>In the framework of the Water In Star-forming regions with <i>Herschel<i/> (WISH) key program, maps in water lines of several outflows from young stars are being obtained, to study the water production in shocks and its role in the outflow cooling. This paper reports the first results of this program, presenting a PACS map of the o-H<sub>2<sub/>O 179 <i>μ<i/>m transition obtained toward the young outflow L1157.<i>Methods. <i/>The 179 <i>μ<i/>m map is compared with those of other important shock tracers, and with previous single-pointing ISO, SWAS, and Odin water observations of the same source that allow us to constrain the H<sub>2<sub/>O abundance and total cooling. <i>Results. <i/>Strong H<sub>2<sub/>O peaks are localized on both shocked emission knots and the central source position. The H<sub>2<sub/>O 179 <i>μ<i/>m emission is spatially correlated with emission from H<sub>2<sub/> rotational lines, excited in shocks leading to a significant enhancement of the water abundance. Water emission peaks along the outflow also correlate with peaks of other shock-produced molecular species, such as SiO and NH<sub>3<sub/>. A strong H<sub>2<sub/>O peak is also observed at the location of the proto-star, where none of the other molecules have significant emission. The absolute 179 <i>μ<i/>m intensity and its intensity ratio to the H<sub>2<sub/>O 557 GHz line previously observed with Odin/SWAS indicate that the water emission originates in warm compact clumps, spatially unresolved by PACS, having a H<sub>2<sub/>O abundance of the order of 10<sup>-4<sup/>. This testifies that the clumps have been heated for a time long enough to allow the conversion of almost all the available gas-phase oxygen into water. The total H<sub>2<sub/>O cooling is ~10<sup>-1<sup/> , about 40% of the cooling due to H<sub>2<sub/> and 23% of the total energy released in shocks along the L1157 outflow.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.715
Threshold uncertainty score0.644

Codex and Gemma teacher scores by category

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)0.0000.000

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 head0.006
GPT teacher head0.210
Teacher spread0.204 · 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 teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designOther design
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

Citations109
Published2010
Admission routes1
Has abstractyes

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