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Record W3127668666

A multi-wavelength study of star formation around HII regions

2002· article· en· W3127668666 on OpenAlexaboutno aff
Jennifer L. Karr

Bibliographic record

VenueTSpace · 2002
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsnot available
Fundersnot available
KeywordsStar (game theory)PhysicsWavelengthAstronomyComputer scienceAstrophysicsOptics
DOInot available

Abstract

fetched live from OpenAlex

The environment of high mass star formation is turbulent and complex. New stars are continually forming while the HII region, stellar winds, and supernovae of the current generation of massive stars destroy the parent molecular cloud. One of the more interesting premises connected with high mass star formation is the possibility that one generation of massive stars and its associated HII region could trigger further star formation as the HII region expands into the surrounding interstellar medium. This thesis uses the Canadian Galactic Plane Survey (a multi-wavelength survey of a portion of the outer Galactic plane) and other archived survey data to study star formation around HII regions, with a particular emphasis on the identification and analysis of evidence for triggered star formation. The use of multi-wavelength data is essential to investigate the ionised, neutral, and molecular components of the gas, the dust, and the population of young stellar objects (YSOs). The survey nature of the data is exploited to study multiple HII regions and star formation in different environments (from energetic to quiescent) in a uniform manner. A variety of HII regions have been explored: W5 and W3/W4, large bright HII regions in the Perseus Arm; W1, a bright HII region in the local arm; LBN 140.77 −1.42, LBN 139.57 +2.70, and LBN 140.07 +1.64, a series of faint HII regions in the Perseus Arm; Sh 2-183, Sh 2-170, Sh 2-173, smaller HII regions at distances of order 2.2 kpc; and Sh 2-185, a nearby HII region. Evidence for direct interactions between the YSOs and molecular gas and the HII region have been found on large and small scales. The interaction between components of the ISM and the distribution and luminosity of star formation has been analysed. Time scales for star formation and triggering have been calculated where possible and the plausibility of triggering evaluated. The nature of star formation outside the neighbourhood of the HII region has been explored and compared with the more active regions. Properties of star formation and molecular clumps in different regions over the sample have been studied, including the areal density of star formation, molecular clump parameters, and the size-linewidth relation.

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: Qualitative · Consensus signal: Qualitative
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.202
Threshold uncertainty score0.355

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 head0.049
GPT teacher head0.297
Teacher spread0.248 · 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 designQualitative
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

Citations0
Published2002
Admission routes1
Has abstractyes

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