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Establishing the accuracy of asteroseismic mass and radius estimates of giant stars – I. Three eclipsing systems at [Fe/H] ∼ −0.3 and the need for a large high-precision sample
Brogaard, K, Hansen, C J, Miglio, A, Slumstrup, D, Frandsen, S, Jessen-Hansen, J, Lund, M N, Bossini, D, Thygesen, A, Davies, G R, Chaplin, W J, Arentoft, T, Bruntt, H, Grundahl, F, Handberg, RVolume:
476
Language:
english
Journal:
Monthly Notices of the Royal Astronomical Society
DOI:
10.1093/mnras/sty268
Date:
May, 2018
File:
PDF, 1.23 MB
english, 2018