The Distribution of Blue Straggler Stars in the Color-Magnitude Diagrams of Old Open Clusters - MESA models

This inlist was used as a template to create the contours of equal fused helium amounts in Figure 3 of Linck and Mathieu 2026a. These models were also used to determine the convective envelope mass fractions used in Figure 2 of Linck and Mathieu 2026b. To recreate these models, vary the initial mass from 0.7 to 2.5 in steps of 0.05 M_Sun. MESA version: r24.03.1 https://doi.org/10.5281/zenodo.10783349MESA SDK version: x86_64-linux-20.3.1 https://doi.org/10.5281/zenodo.3706650Run on Docker: https://doi.org/10.5281/zenodo.10905784