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Meredith L. Rawls edited figures/adaptedfig1/caption.tex
almost 10 years ago
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Replace this text with your caption Solar-like oscillation spectra of nine stars observed by \emph{Kepler}. Redder colors indicate later evolutionary phases, and correspondingly lower surface gravity. All stars shown have masses close to $1~M_{\odot}$. Those in the right panel are from short-cadence \emph{Kepler} data ($\sim 1$ min), and those on the left are from long-cadence mode ($\sim 30$ min). The top two stars on the right are main-sequence stars, the third and fourth stars down are subgiants, and the bottom star lies at the base of the RGB. The top two stars on the left are first-ascent RGB stars, and the bottom two are, respectively, RGB and RC stars that share similar surface properties. Figure adapted from \citet{cha13}.
