A seismic and gravitationally bound double star observed by Kepler. Implication for the presence of a convective core
Context. Solar-like oscillations have been observed by Kepler and CoRoT in many solar-type stars, thereby providing a way to probe stars using asteroseismology. Aims: The derivation of stellar parameters has usually been done with single stars. The aim of the paper is to derive the stellar parameters of a double-star system (HIP 93511), for which
Appourchaux, T. et al.
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2015