Rotating single star models for the Galaxy computed with MESA

The model dataset described/employed in the paper "Boron depletion in Galactic early B-type stars reveals two different main sequence star populations" by Harim Jin , Norbert Langer, Daniel J. Lennon , and Charles R. Proffitt (2024). single_star_models A grid of rotating single star models for Z=0.0154 computed with MESA The models are named by their initial masses in log (in solar mass) and initial rotational velocities (in km/s). E.g., 1.080_200 is a 12 Msun with an initial velocity of 200 km/s. Initial masses: 5-40 Msun Initial rotational velocities: 0-600 km/s (or up to break-up) MESA_input_data MESA input data files to reproduce the single star models Works with MESA version of 10398 and MESA SDK version of x86_64-linux-20180822.