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Dennis edited We_quantify_the_mass_dependent__.tex
almost 9 years ago
Commit id: 054bfa5b5a31fdcad677b5d0fcca9d52b9b8c4b3
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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 low-mass hydrogen-core burning
stars. % stars \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
% magnetic fields that survive after hydrogen burning ceases in the core.