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Paper detail

Red Giants observed with CoRoT

Observations of red (G-K)-giant stars with the CoRoT satellite provide unprecedented information on the stochastically excited oscillations in these stars. The long time series of nearly uninterrupted high-cadence and high-precision photometry revealed the presence of non-radial modes with long lifetimes, which opens the possibility to perform asteroseismology on these stars. Also, the large number of red giants, for which solar-like oscillations are now observed, allows for a more statistical investigation of the characteristics of solar-like oscillations in red giants.

preprint2010arXivOpen access
S. HekkerJ. De RidderF. BaudinC. BarbanF. CarrierA. P. HatzesT. KallingerW. W. Weiss
astro-ph.SR
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S. HekkerJ. De RidderF. BaudinC. BarbanF. CarrierA. P. HatzesT. KallingerW. W. Weiss

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