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Record W2607177416 · doi:10.3847/1538-4357/aa6a1e

The Correlation between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia Era

2017· article· en· W2607177416 on OpenAlexfundno aff
Jamie Tayar, Garrett Somers, Marc H. Pinsonneault, Dennis Stello, Alexey Mints, Jennifer A. Johnson, O. Zamora, D. A. García–Hernández, Claudia Maraston, Aldo Serenelli, Carlos Allende Prieto, Fabienne A. Bastien, Sarbani Basu, Jonathan C. Bird, Roger E. Cohen, Kátia Cunha, Y. Elsworth, R. A. García, L. Girardi, S. Hekker, Jon A. Holtzman, S. Mathur, Szabolcs Mészáros, B. Mosser, Matthew Shetrone, V. Silva Aguirre, Keivan G. Stassun, Guy S. Stringfellow, Gail Zasowski, Alexandre Roman–Lopes

Bibliographic record

VenueThe Astrophysical Journal · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratorySmithsonian Astrophysical ObservatoryScience and Technology Facilities CouncilUniversity of Colorado BoulderInstituto de Astrofísica de CanariasOffice of ScienceMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikNemzeti Kutatási Fejlesztési és Innovációs HivatalMinistério da Ciência, Tecnologia e InovaçãoMinisterio de Economía y CompetitividadCentre National d’Etudes SpatialesGeneralitat de CatalunyaUniversity of OxfordYork UniversityUniversidad Nacional Autónoma de MéxicoMagyar Tudományos AkadémiaSpace Telescope Science InstituteVillum FondenComisión Nacional de Investigación Científica y TecnológicaNational Aeronautics and Space AdministrationStellar Astrophysics CentreDanmarks GrundforskningsfondLeibniz-GemeinschaftUniversity of Notre DameOhio State UniversityNational Research FoundationCarnegie Mellon UniversityAlfred P. Sloan FoundationUniversity of WashingtonJohns Hopkins UniversityUniversity of UtahCarnegie Institution of WashingtonNational Science FoundationSmithsonian InstitutionU.S. Department of EnergyNew Mexico State UniversityUniversity of PortsmouthVanderbilt UniversityNational Research, Development and Innovation OfficeScience Mission DirectorateYale University
KeywordsMetallicityPhysicsAstrophysicsMixing (physics)Convective mixingRed-giant branchStarsRed giantStellar massConvectionAstronomyStar formationMeteorology

Abstract

fetched live from OpenAlex

Abstract In the updated APOGEE- Kepler catalog, we have asteroseismic and spectroscopic data for over 3000 first ascent red giants. Given the size and accuracy of this sample, these data offer an unprecedented test of the accuracy of stellar models on the post-main-sequence. When we compare these data to theoretical predictions, we find a metallicity dependent temperature offset with a slope of around 100 K per dex in metallicity. We find that this effect is present in all model grids tested, and that theoretical uncertainties in the models, correlated spectroscopic errors, and shifts in the asteroseismic mass scale are insufficient to explain this effect. Stellar models can be brought into agreement with the data if a metallicity-dependent convective mixing length is used, with Δ α ML,YREC ∼ 0.2 per dex in metallicity, a trend inconsistent with the predictions of three-dimensional stellar convection simulations. If this effect is not taken into account, isochrone ages for red giants from the Gaia data will be off by as much as a factor of two even at modest deviations from solar metallicity ([Fe/H] = −0.5).

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)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.286
Threshold uncertainty score0.998

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0030.000
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 head0.034
GPT teacher head0.277
Teacher spread0.243 · 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.

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

Citations126
Published2017
Admission routes1
Has abstractyes

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