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Record W1985342635 · doi:10.1088/0004-637x/708/2/1002

THE INITIAL CONDITIONS OF CLUSTERED STAR FORMATION. II. N<sub>2</sub>H<sup>+</sup>OBSERVATIONS OF THE OPHIUCHUS B CORE

2009· article· en· W1985342635 on OpenAlexaff
Rachel Friesen, James Di Francesco, Yoshito Shimajiri, Shigehisa Takakuwa

Bibliographic record

VenueThe Astrophysical Journal · 2009
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsNational Research Council CanadaUniversity of VictoriaHerzberg Institute of Astrophysics
Fundersnot available
KeywordsOphiuchusAstrophysicsPhysicsMolecular cloudProtostarLine (geometry)Star formationAstronomyStarsGeometry

Abstract

fetched live from OpenAlex

We present a Nobeyama 45 m Radio Telescope map and Australia Telescope Compact Array pointed observations of N 2 H + 1-0 emission toward the clustered, low-mass star-forming Oph B Core within the Ophiuchus molecular cloud. We compare these data with previously published results of high-resolution NH 3 (1,1) and (2,2) observations in Oph B. We use 3D clumpfind to identify emission features in the single-dish N 2 H + map, and find that the N 2 H + "clumps" match well similar features previously identified in NH 3 (1,1) emission, but are frequently offset to clumps identified at similar resolution in 850 μm continuum emission. Wide line widths in the Oph B2 sub-Core indicate that non-thermal motions dominate the Core kinematics, and remain transonic at densities n ∼ 3 × 10 5 cm −3 with large scatter and no trend with N (H 2 ). In contrast, non-thermal motions in Oph B1 and B3 are subsonic with little variation, but also show no trend with H 2 column density. Over all of Oph B, non-thermal N 2 H + line widths are substantially narrower than those traced by NH 3 , making it unlikely NH 3 and N 2 H + trace the same material, but the v LSR of both species agree well. We find evidence for accretion in Oph B1 from the surrounding ambient gas. The NH 3 /N 2 H + abundance ratio is larger toward starless Oph B1 than toward protostellar Oph B2, similar to recent observational results in other star-forming regions. The interferometer observations reveal small-scale structure in N 2 H + 1-0 emission, which are again offset from continuum emission. No interferometric N 2 H + emission peaks were found to be coincident with continuum clumps. In particular, the ∼1 M ☉ B2-MM8 clump is associated with an N 2 H + emission minimum and surrounded by a broken ring-like N 2 H + emission structure, suggestive of N 2 H + depletion. We find a strong general trend of decreasing N 2 H + abundance with increasing N (H 2 ) in Oph B which matches that found for NH 3 .

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)0.001
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 score0.011
Threshold uncertainty score0.022

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.028
GPT teacher head0.263
Teacher spread0.235 · 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

Citations54
Published2009
Admission routes1
Has abstractyes

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