deletions | additions       diff --git a/Speculations_Forward_look_Our_results__.tex b/Speculations_Forward_look_Our_results__.tex  index 9fc442d..32a3228 100644  --- a/Speculations_Forward_look_Our_results__.tex  +++ b/Speculations_Forward_look_Our_results__.tex 
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mixing processes in their interiors including thermohaline mixing, which does not occur in a fraction of red giants \cite{Charbonnel_2007}.  %The strong dynamo-generated fields reported here have survived from hydrogen-core burning to hydrogen-shell burning.   After hydrogen-shell burning, intermediate-mass stars burn helium in their cores. Suppressed dipole modes in red clump stars will reveal whether the fields survive until helium-core burning, and whether they can account for magnetic fields observed in stellar remnants such as white dwarfs.   CAN WE SAY MORE? TIM THOUGHT THIS WAS A WEAK ENDING.  %[Suppressed stars seem not to show significant surface fields beyond normal  %(Ballot in prep.) RAFA HAVE YOU HEARD ANYTHING FROM JEROME HOW FAR HE  %IS? CAN WE REFER TO THIS?]