Kepler asteroseismology of red-giant stars

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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To appear in Proceedings of the 61st Fujihara Seminar: Progress in solar/stellar physics with helio- and asteroseismology. H.

Scientific paper

The Kepler mission, launched in March 2009, has revolutionized asteroseismology, providing detailed observations of thousands of stars. This has allowed in-depth analysis of stars ranging from compact hot subdwarfs to red giants, and including the detection of solar-like oscillations in hundreds of stars on or near the main sequence. Here I mainly consider solar-like oscillations in red giants, where Kepler observations are yielding results of a perhaps unexpected richness. In addition to giving a brief overview of the observational and numerical results for these stars, I present a simple analysis which captures some of the properties of the observed frequencies.

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