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Record W1505005917 · doi:10.1086/324447

The Disk and Environment of the Herbig B[CLC]e[/CLC] Star HD 100546

2001· article· en· W1505005917 on OpenAlex
C. A. Grady, Elisha Polomski, Th. Henning, B. Stecklum, B. E. Woodgate, C. M. Telesco, R. K. Piña, T. R. Gull, A. Boggess, Charles W. Bowers, F. C. Bruhweiler, Mark Clampin, A. C. Danks, R. F. Green, Sara R. Heap, J. B. Hutchings, E. B. Jenkins, C. L. Joseph, M. E. Kaiser, Randy A. Kimble, S. B. Kraemer, D. Lindler, Jeffrey L. Linsky, S. P. Maran, H. W. Moos, P. Plait, F. L. Roesler, J. G. Timothy, D. Weistrop

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.

Bibliographic record

VenueThe Astronomical Journal · 2001
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsDominion Astrophysical Observatory
Fundersnot available
KeywordsPhysicsAstrophysicsHerbig Ae/Be starSpace Telescope Imaging SpectrographAstronomyBe starStar (game theory)BrightnessTelescopeStarsSpitzer Space TelescopeObservatoryAdvanced Camera for SurveysEnvelope (radar)Surface brightnessStar formationHubble space telescopeT Tauri starK-type main-sequence starGalaxy

Abstract

fetched live from OpenAlex

Coronagraphic imaging of the nearest Herbig Be star with the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope, Ks (2.15 μm) imaging with ADONIS at the 3.6 m telescope at La Silla, and mid-infrared imaging with OSCIR using the 4 m Blanco Telescope at Cerro Tololo Inter-American Observatory confirm the detection of the disk reported by Pantin et al. and map the disk out to 5'' (∼515 AU) in the optical and at Ks. While the source is unresolved at 10 and 18 μm, it can be traced to 15 at 11.7 μm. We confirm the change in the radial dependence of the disk surface brightness near 27 seen at 1.6 μm by Augereau et al. at Ks. No such break in the power law is seen in the optical. The STIS data reveal spiral dark lane structure, making HD 100546 the third near–zero-age main-sequence Herbig Ae/Be star with structure more than 100 AU from the star. We also optically detect a low surface brightness envelope extending 10'' (1000 AU) from the star, in addition to nebulosity, which is probably associated with DC 292.6-7.9. The survival of the envelope through essentially the entire pre–main-sequence lifetime of the star, coupled with the absence of physical companions within 1500 AU of the star, suggests that envelope lifetimes owe more to the star-forming environment than to mass-loss activity from the Herbig Ae/Be star.

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.

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: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.546
Threshold uncertainty score0.631

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 studies0.0010.000
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 head0.007
GPT teacher head0.197
Teacher spread0.190 · 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