What's Their Age Again? A Blue-Straggler Merger Scenario in the $\gamma$ Persei Binary System

Stellar evolutionary tracks generated with MESA (v23.05.1) for the paper ``What's Their Age Again? A Blue-Straggler Merger Scenario in the $\gamma$ Persei Binary System`` This repository contains history files for the components (component_1.tar.gz and component_2.tar.gz) of the $\gamma$ Persei system. The simulations cover a range of initial masses and metallicities for both stars: the primary component spans $3.2 - 3.8,M_\odot$ with [Fe/H] = -0.29, -0.19, -0.09, while the secondary spans $2.2 - 2.6,M_\odot$ with [Fe/H] = -0.30, -0.20, -0.10. Convection and mixing are modeled using various mixing-length parameters ($\alpha_\mathrm{MLT} = 1.5 - 2.5$) and exponential overshoot schemes with three overshoot settings.