Simulations predict that detectable two-star pulsators have near-equal initial masses, that double red-clump binaries are absent below about 500 solar radii, and that roughly one percent of red giants have gained or lost significant mass.
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DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations
Simulations predict that detectable two-star pulsators have near-equal initial masses, that double red-clump binaries are absent below about 500 solar radii, and that roughly one percent of red giants have gained or lost significant mass.