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Record W2130527029 · doi:10.1088/0004-637x/773/2/102

<i>HERSCHEL</i>REVEALS MASSIVE COLD CLUMPS IN NGC 7538

2013· article· en· W2130527029 on OpenAlexaff
C. Fallscheer, Michael A. Reid, James Di Francesco, P. G. Martin, T. Hill, M. Hennemann, Q. Nguyễn Lương, F. Motte, A. Men’shchikov, Ph. André, D. Ward–Thompson, M. J. Griffin, J. M. Kirk, V. Könyves, K. L. J. Rygl, Sarah Sadavoy, M. Sauvage, N. Schneider, L. D. Anderson, M. Benedettini, J.-P. Bernard, Adam Ginsburg, S. Molinari, D. Polychroni, A. Rivera-Ingraham, H. Roussel, L. Testi, G. J. White, Jonathan P. Williams, C. D. Wilson, M. Wong, A. Zavagno

Bibliographic record

VenueThe Astrophysical Journal · 2013
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of British ColumbiaNational Research Council CanadaCanadian Institute for Theoretical AstrophysicsMcMaster UniversityUniversity of TorontoUniversity of Victoria
FundersScience and Technology Facilities Council
KeywordsSpire (mollusc)PhysicsAstrophysicsStarsLuminosityStar formationHigh massInfraredAstronomyYoung stellar objectCover (algebra)Far infraredGalaxy

Abstract

fetched live from OpenAlex

We present the first overview of the Herschel observations of the nearby high-mass star-forming region NGC 7538, taken as part of the Herschel imaging study of OB young stellar objects (HOBYS) Key Programme. These PACS and SPIRE maps cover an approximate area of one square degree at five submillimeter and far-infrared wavebands. We have identified 780 dense sources and classified 224 of those. With the intention of investigating the existence of cold massive starless or class 0-like clumps that would have the potential to form intermediate- to high-mass stars, we further isolate 13 clumps as the most likely candidates for follow-up studies. These 13 clumps have masses in excess of 40 M ☉ and temperatures below 15 K. They range in size from 0.4 pc to 2.5 pc and have densities between 3 × 10 3 cm −3 and 4 × 10 4 cm −3 . Spectral energy distributions are then used to characterize their energetics and evolutionary state through a luminosity–mass diagram. NGC 7538 has a highly filamentary structure, previously unseen in the dust continuum of existing submillimeter surveys. We report the most complete imaging to date of a large, evacuated ring of material in NGC 7538 which is bordered by many cool sources.

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 score0.031
Threshold uncertainty score0.061

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)0.0020.001

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 head0.009
GPT teacher head0.228
Teacher spread0.219 · 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

Citations32
Published2013
Admission routes1
Has abstractyes

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Same venueThe Astrophysical JournalSame topicAstrophysics and Star Formation StudiesFrench-language works237,207