deletions | additions       diff --git a/sectionAcknowledgmen.tex b/sectionAcknowledgmen.tex  index 567a01f..ca23fac 100644  --- a/sectionAcknowledgmen.tex  +++ b/sectionAcknowledgmen.tex 
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change_net = .true.   new_net_name = 'mesa_201.net'  \end{verbatim}  Although our choices affect the precise details of the model (e.g., He core mass), the general features of our model are robust. For instance, We we  find that a 14 $M_\odot$ model with less overshoot produces very similar results. Our low-mass models explode as red supergiants, and they undergo convective core C-burning, followed by shell C-burning, core O/Ne-burning, shell O-burning, core Si-burning, shell-Si burning, and then CC. The approximate convective properties (as described by MLT) are not strongly affected by model parameters. Since these properties are most important for IGW AM transport, we argue that the general features of IGWs described in this work are fairly robust against uncertain parameters in our massive star models.