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- W2126982983 abstract "Context. Subdwarf B pulsators exhibit pressure (p) and/or gravity (g) modes. Their frequency spectra range from very simple, with few frequencies, to very rich, with more than fifty peaks in some cases. Balloon09 is a hybrid pulsating subdwarf B, showing a great number of p- and g-modes including triplet and quintuplet-like structures, which are interpreted as p-mode frequency splittings caused by stellar rotation. Photometric observations undertaken in two subsequent years revealed a change in these rotational splittings of 0.24 − 0.58 μHz/yr." @default.
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- W2126982983 date "2011-11-01" @default.
- W2126982983 modified "2023-10-17" @default.
- W2126982983 title "Angular momentum transfer between oscillations and rotation in subdwarf B hybrid pulsators" @default.
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