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Record W2796869514 · doi:10.1093/mnras/sty1011

The Gaia-ESO Survey: evidence of atomic diffusion in M67?

2018· article· en· W2796869514 on OpenAlexaff
Clio Bertelli Motta, A. Pasquali, J. Richer, G. Michaud, M. Salaris, A. Bragaglia, L. Magrini, S. Randich, E. K. Grebel, V. Adibekyan, S. Blanco-Cuaresma, A. Drazdauskas, Xiaoting Fu, Sarah L. Martell, G. Tautvaiśienė, G. Gilmore, E. J. Alfaro, T. Bensby, E. Flaccomio, S. E. Koposov, A. J. Korn, A. C. Lanzafame, R. Smiljanić, A. Bayo, G. Carraro, Andrew R. Casey, F. Damiani, E. Franciosini, U. Heiter, A. Hourihane, P. Jofré, C. Lardo, J. Lewis, L. Monaco, L. Morbidelli, G. G. Sacco, S. G. Sousa, C. C. Worley, S. Zaggia

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversité de Montréal
FundersEuropean Social FundFundação para a Ciência e a TecnologiaEuropean Science FoundationLietuvos Mokslo TarybaSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungKnut och Alice Wallenbergs StiftelseDeutsche ForschungsgemeinschaftEuropean CommissionScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaLeverhulme TrustNational Aeronautics and Space AdministrationMinisterio de Economía y CompetitividadNational Science Foundation
KeywordsPhysicsAstrophysicsMetallicityOpen clusterStarsChemical evolutionCluster (spacecraft)Stellar evolutionAstronomyStar clusterRed-giant branchMass segregationSpectral line

Abstract

fetched live from OpenAlex

Investigating the chemical homogeneity of stars born from the same molecular cloud at virtually the same time is very important for our understanding of the chemical enrichment of the interstellar medium and with it the chemical evolution of the Galaxy.One major cause of inhomogeneities in the abundances of open clusters is stellar evolution of the cluster members.In this work, we investigate variations in the surface chemical composition of member stars of the old open cluster M67 as a possible consequence of atomic diffusion effects taking place during the main-sequence phase.The abundances used are obtained from high-resolution UVES/FLAMES spectra within the framework of the Gaia-ESO Survey.We find that the surface abundances of stars on the main sequence decrease with increasing mass reaching a minimum at the turnoff.After deepening of the convective envelope in sub-giant branch stars, the initial surface abundances are restored.We found the measured abundances to be consistent with the predictions of stellar evolutionary models for a cluster with the age and metallicity of M67.Our findings indicate that atomic diffusion poses a non-negligible constraint on the achievable precision of chemical tagging methods.

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 score0.008
Threshold uncertainty score0.017

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
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 head0.015
GPT teacher head0.242
Teacher spread0.228 · 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
Published2018
Admission routes1
Has abstractyes

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