deletions | additions       diff --git a/We_quantify_the_mass_dependent__.tex b/We_quantify_the_mass_dependent__.tex  index d1fbb1d..60a5e05 100644  --- a/We_quantify_the_mass_dependent__.tex  +++ b/We_quantify_the_mass_dependent__.tex 
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burning phase \citep{Kippenhahn_1990}.  We believe this shows evidence for the establishment of  convectively driven dynamos in the cores of hydrogen-core burning  stars that are only 10-20\% more massive than the Sun \citep{Charbonneau_2001,MacGregor_2003,Brun_2005}. [THE SENTENCE BEFORE AND   AFTER DONT REALLY WORK TOGTHER BUT I FEEL WE NEED TO SAY SOMEHOW WHAT IS SAID   IN THE FOLLOWING SENTENCE] The resulting strong magnetic fields   survives after core burning ceases making them observable in the red giant phase.  % The gradual increase in suppression may result from the increasing size of  % the convective core in more massive stars, which generates stronger  % magnetic fields that survive after hydrogen burning ceases in the core.