deletions | additions       diff --git a/section_Tides_and_stuff_In__.tex b/section_Tides_and_stuff_In__.tex  index cb45ad9..f0a810c 100644  --- a/section_Tides_and_stuff_In__.tex  +++ b/section_Tides_and_stuff_In__.tex 
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\section{Tides and stuff}  In the absence of external influences, all evolved giant stars with a convective outer layer should exhibit solar-like oscillations. However, that is clearly not the case for three of the seven RG/EBs in our sample. \citet{gau14} proposed that stronger tidal interactions from short-period binaries and increased magnetic activity on spotty giants are linked to absent or damped solar-like oscillations.  Now we examine that... with that. With  MESA models, a quantitative comparison of how active each star is, and a quantitative estimation of tidal forces being exerted in each binary over its lifetime. 123 1,2,3,  go.