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Record W2954420793 · doi:10.1093/mnrasl/slz085

SDSS-IV MaNGA: stellar population gradients within barred galaxies

2019· article· en· W2954420793 on OpenAlexfundno aff
Amelia Fraser-McKelvie, M. R. Merrifield, Alfonso Aragón‐Salamanca, Thomas Peterken, Karen L. Masters, Coleman Krawczyk, Brett H. Andrews, J. H. Knapen, Sandor Kruk, Adam Schaefer, Rebecca Smethurst, Rogério Riffel, Joel R. Brownstein, Niv Drory

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society Letters · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratorySmithsonian Astrophysical ObservatoryScience and Technology Facilities CouncilHorizon 2020 Framework ProgrammeUniversity of Colorado BoulderInstituto de Astrofísica de CanariasOffice of ScienceMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikUniversidad Nacional Autónoma de MéxicoBanco Bilbao Vizcaya ArgentariaMinistério da Ciência, Tecnologia e InovaçãoLiverpool John Moores UniversityConselho Nacional de Desenvolvimento Científico e TecnológicoMinisterio de Economía y CompetitividadUniversity of OxfordLeverhulme TrustYork UniversityFundação de Amparo à Pesquisa do Estado do Rio Grande do SulSavannah River Operations Office, U.S. Department of EnergyCarnegie Mellon UniversityUniversity of WashingtonJohns Hopkins UniversityLeibniz-GemeinschaftUniversity of Notre DameFundación BBVAOhio State UniversityCarnegie Institution of WashingtonNew Mexico State UniversityUniversity of PortsmouthVanderbilt UniversityYale UniversityEuropean CommissionU.S. Department of EnergySmithsonian Institution
KeywordsGalaxyStellar populationAstrophysicsAstronomyPhysicsStar formation

Abstract

fetched live from OpenAlex

ABSTRACT Bars in galaxies are thought to stimulate both inflow of material and radial mixing along them. Observational evidence for this mixing has been inconclusive so far, however, limiting the evaluation of the impact of bars on galaxy evolution. We now use results from the MaNGA integral field spectroscopic survey to characterize radial stellar age and metallicity gradients along the bar and outside the bar in 128 strongly barred galaxies. We find that age and metallicity gradients are flatter in the barred regions of almost all barred galaxies when compared to corresponding disc regions at the same radii. Our results re-emphasize the key fact that by azimuthally averaging integral field spectroscopic data one loses important information from non-axisymmetric galaxy components such as bars and spiral arms. We interpret our results as observational evidence that bars are radially mixing material in galaxies of all stellar masses, and for all bar morphologies and evolutionary stages.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.122
Threshold uncertainty score0.896

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 science0.0010.000
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 head0.005
GPT teacher head0.179
Teacher spread0.175 · 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 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

Citations41
Published2019
Admission routes1
Has abstractyes

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