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Jim Fuller edited sectionAcknowledgmen.tex
about 9 years ago
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Our stellar models are constructed using the MESA stellar evolution code \citep{paxton:11,paxton:13}, version 6794. The models are run using the following inlist controls file.
\begin{multicol}{2} \begin{multicols}{2}
\begin{verbatim}
\& star_job
...
/ ! end of controls namelist
\end{verbatim}
\end{multicol} \end{multicols}
The most important feature of this model is that it contains significant convective overshoot, especially above convective zones. It is non-rotating, thus there is no rotational mixing.