Transitory tidal heating events and their impact on cluster isochrones

<p>MESA inlists and run_star_extras.f90 for simulating transitory tidal heating events (Arthur et al., 2024). Uses MESA version r15140 and MESA SDK version x86_64-linux-20.12.1.</p> <p>inlist_start: evolve a low-mass star to ZAMS</p> <p>inlist_after_zams: evolve a low-mass star from ZAMS to 3.95 giga years (age of M67 cluster)</p> <p>inlist_near_tams: add heating to the stellar envelope using heating rates from TIDESnnv models</p> <p>history_columns.list</p> <p>profile_columns.list</p> <p>run_star_extras.f90: envelope heating routine interpolating TIDESnnv models.</p> <p>Inlists and run_star_extras.f90 were adapted from MIST resources (Choi et al., 2016; Dotter et al 2016) and use tailored convection parameters described in these works. Available from <a href="https://waps.cfa.harvard.edu/MIST">https://waps.cfa.harvard.edu/MIST</a></p> <p><br>Heating rates come from tailored <a href="../doi/10.5281/zenodo.10799021">TIDESnnv</a> (Tidal Interactions with Dissipation of Energy due to Shear version nvv) models.</p>