Example input files for Wolf-Rayet star models in paper "Tidal Spin-up of Black Hole Progenitor Stars"

The files here show example input files for the models in the paper "Tidal Spin-up of Black Hole Progenitor Stars" by Ma &amp; Fuller (2023). File "inlist_MS" and "inlist_WR" show MESA inlists to set up a Wolf-Rayet star model of 10 solar-masses (model 3 in Ma &amp; Fuller 2023, Table 1).<br> We used MESA version r12778 for our calculation.<br> Specifically, "inlist_MS" starts a stellar model at zero-age main-sequence (ZAMS), and evolves it to the end of core hydrogen depletion.<br> After resuming the model from a photo file, "inlist_WR" turns on artificial mass-loss ("relax_mass" and "new_mass") to remove its hydrogen envelope, and then evolves the model throughout the helium burning Wolf-Rayet phase, until the end of core helium depletion.<br> During this phase, pulsation data are also created by MESA ("write_pulse_data_with_profile = .true."). <br> File "gyre.in" is an example GYRE input file to solve for oscillation modes in the established Wolf-Rayet star models.<br> We used GYRE version 6.0.1 for our calculation.