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Paper: g-Mode Pulsators along the Horizontal Branch
Volume: 452, Fifth Meeting on Hot Subdwarf Stars and Related Objects
Page: 251
Authors: O'Toole, S. J.
Abstract: Kepler has been a boon for asteroseismology, detecting oscillations in many different stars across the HR diagram. High precision data over long timescales has allowed us to detect many g-mode oscillations in sdB stars in particular, but also in other Horizontal Branch stars. Here I point out the very similar g-mode period spacings detected in sdB and Red Clump stars, and discuss what we can learn by comparing oscillations in these objects.
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