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How accurate are stellar ages based on stellar models? II. The impact of asteroseismology
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Accurate and precise stellar ages are best determined for stars which are strongly observationally constrained, that is which are intrinsically oscillating. We review here the seismic diagnostics which are sensitive to stellar ages and provide some illustrating examples of seismically age-dated stars.
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Uniform characterisation of an ensemble of main-sequence benchmark stars: effect of Gaia-based data on grid search models
Adding Gaia-based luminosities to grid-based asteroseismic modelling improves mass precision for main-sequence benchmarks but leaves radii systematically underestimated, and 1 per cent precise interferometric radii wo...
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