Testing the Asteroseismic Scaling Relations for Red Giants with Eclipsing Binaries Observed by Kepler
Given the potential of ensemble asteroseismology for understanding fundamental properties of large numbers of stars, it is critical to determine the accuracy of the scaling relations on which these measurements are based. From several powerful validation techniques, all indications so far show that stellar radius estimates from the asteroseismic
Gaulme, P. et al.
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2016