Meredith L. Rawls edited abstract.tex  almost 8 years ago

Commit id: 19af2b37d9c36f51661a3d918b4b4b2bfd3d437c

deletions | additions      

       

Of the 18 known red giants in eclipsing binaries (RG/EBs), four do not show solar-like oscillations. These four also have the most signs of magnetic activity and tidal forces. A handful of the rest show suppressed oscillation modes with moderate levels of magnetism and tides.  This paper uses \emph{Kepler} light curves, high-resolution spectra, and stellar evolution modeling to demonstrate this trend and discuss the physical mechanisms responsible. Comments welcome. [Abstract placeholder]