deletions | additions       diff --git a/SETTING_UP_FOR_THE_PRESENTATION__.tex b/SETTING_UP_FOR_THE_PRESENTATION__.tex  index f46cc1b..463efa7 100644  --- a/SETTING_UP_FOR_THE_PRESENTATION__.tex  +++ b/SETTING_UP_FOR_THE_PRESENTATION__.tex 
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find stars with significantly suppressed dipole modes (bottom panels).  % a phenomena previously observerved in X red giants  % [refMosser2012LargeKepler] and a subgiant star [ref Droopy].   Suppressed dipole modes were first observed in a few dozen red giant  stars \citep{Mosser_2011}, \citep{Mosser_2011,Garc_a_2014},  and we find several hundred more stars. The cause of thissuppression  phenomenon has been puzzling until recent theoretical work, which shows that the suppression can be explained if waves entering the stellar core are prevented from returning to the envelope. %, preventing the establishment of standing waves.   This occurs in the presence of strong magnetic fields in the core, giving rise to a ``magnetic greenhouse'' effect that efficiently traps wave energy leaking into the core (Fuller et al. 2015).