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Paper: Kepler Asteroseismology of Red-giant Stars
Volume: 462, Progress in Solar/Stellar Physics with Helio- and Asteroseismology
Page: 503
Authors: Christensen-Dalsgaard, J.
Abstract: The Kepler mission, launched in March 2009, has revolutionized asteroseismology, providing detailed observations of thousands of stars. This has allowed in-depth analyses 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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