Three sdB stars show sharp core glitches located at larger buoyancy radius and with larger amplitudes than those in helium-core-burning red giants, hinting at more extensive core-boundary mixing.
S., Van Grootel , V., stensen , R
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Probing the Cores of Subdwarf B Stars: How do They Compare to Cores in Helium Core-Burning Red Giants?
Three sdB stars show sharp core glitches located at larger buoyancy radius and with larger amplitudes than those in helium-core-burning red giants, hinting at more extensive core-boundary mixing.