Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity

<p>Model data and input files (inlists) used to compute MESA binary models to paper<br> &quot;Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity&quot;<br> (<a href="https://ui.adsabs.harvard.edu/abs/2021arXiv211110271K/abstract">ADS link</a>)<br> MESA version&nbsp;r11554.<br> <br> The data consists of stellar tracks of the primary (donor) star. Provided are MESA history.data files and the final MESA model of the primary (terminated at core-He depletion).<br> <br> The data for solar metallicity models is also available on request.<br> &nbsp;</p>