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Meredith L. Rawls edited untitled.tex
over 8 years ago
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\textit{Oh, an empty article!} \section{Introduction}\label{intro}
\begin{itemize}
\item Why RG/EBs are useful
\item Why we care about understanding when solar-like oscillations can happen
\item How studying tides and stellar activity can help
\end{itemize}
The combination of \emph{Kepler} light curves, radial velocities, multi-band photometry, and high-resolution optical spectra allows us to thoroughly characterize the physical properties of both stars in each binary. To better understand the relationship between tidal forces, stellar activity, and solar-like oscillations, we study a subset of RG/EBs that include binaries with short and long orbital periods (< 100 days and > 100 days, respectively), and red giants that exhibit and lack solar-like oscillations. An overview of the six systems is presented in Table REFERENCE HERE.
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