What it is
In this study, we report three systems-24 Boo b, HD 12648 b, and TYC 4282-605-1 b-whose host stars are confirmed red-clump giants through asteroseismology, showing that each has already undergone dramatic expansion and contraction following helium ignition.
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Filed underStellar, planetary, and galactic studies, History and Developments in Astronomy, Astronomy and Astrophysical Research