Bridging the Gap between Intermediate and Massive Stars II: $M_{\text{mas}}$ for the most metal--rich stars and implications for Fe CCSNe rates

Working directory to accompany:

"Bridging the Gap between Intermediate and Massive Stars II: $M_{\text{mas}}$ for the most metal--rich stars and implications for Fe CCSNe rates"

G. C. Cinquegrana, M. Joyce and A. Karakas

This directory is designed to run metal-rich models from the zero age main sequence to core carbon depletion. Currently, it is set to run a 9.4Msun model with Z=0.08. Initial mass and metallicity parameters are set in 'inlist_mass_Z'. You will also need to adjust the lower H limit in 'inlist_to_zams' when changing initial metallicity (values are commented in that file).