Material needed to reproduce the profiles of semiconvective and overshooting models during core He burning in a 3Msun, as in figure 11.
This archive contains the inlist required to run the calculations used for producing figure 12 (Thermohaline Mixing on the RGB for a rotating 1Msun). Content in the preamble gives a few more details and the MESA version #. The history.data and profile.data files are also provided.
Archives with the material needed to reproduce figures 13-15 in section 4.3.