deletions | additions       diff --git a/We_quantify_the_mass_dependent__.tex b/We_quantify_the_mass_dependent__.tex  index f8fed02..69bd938 100644  --- a/We_quantify_the_mass_dependent__.tex  +++ b/We_quantify_the_mass_dependent__.tex 
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1.5\msun, and a drop beyond 2.0\msun.   The onset of suppression beyond 1.1\msun, coincides with the mass above  which stars are thought to form convective cores during their hydrogen-core  burning phase[REF]. phase \citep{Kippenhahn_1990}.  We believe this shows evidence for the establishment of  convectively driven convectively-driven  dynamos in the cores of low-mass hydrogen-core burning stars [REF CharbonneauMacGregor01,MacgregorCassinelli03Brun05].   %  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. %  [Jim/Matteo elaborate?]