g-Mode Pulsators along the Horizontal Branch

Details g-Mode Pulsators along the Horizontal Branch g-Mode Pulsators along the Horizontal Branch

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aspc..452..251o&link_type=abstract

Fifth Meeting on Hot Subdwarf Stars and Related Objects, ASP Conference Series Vol. 452, proceedings of a workshop held at Stell

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Scientific paper

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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