deletions | additions       diff --git a/We_quantify_the_mass_dependent__.tex b/We_quantify_the_mass_dependent__.tex  index 2b22244..a21953d 100644  --- a/We_quantify_the_mass_dependent__.tex  +++ b/We_quantify_the_mass_dependent__.tex 
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which stars are thought to form convective cores during their hydrogen-core  burning phase \citep{Kippenhahn_1990}.  We believe this shows evidence for the establishment of  convectively-driven convectively driven  dynamos in the cores of hydrogen-core hydrogen core  burning stars that are that are only 10-20\% more massive than the Sun \citep{Charbonneau_2001,MacGregor_2003,Brun_2005}.   % The gradual increase in suppression may result from the increasing size of  % the convective core in more massive stars, which generates stronger