MESA inlists and data for "On the origin of carbon- and oxygen-rich hot subdwarfs: an sdB merger scenario"

The uploaded files contain the MESA (version 24.08.01) evolutionary data used in the paper "On the origin of carbon- and oxygen-rich hot subdwarfs: an sdB merger scenario". Two data sets are provided, corresponding to the single-star and binary-star modules calculated with MESA in this work. The single-star module was used to simulate the two formation channels proposed in this paper: the sdB + sdB merger and the He WD + sdB merger. The binary-star module was employed to evolve the mass transfer process in the double sdB binary systems. Each set includes the initial models, the inlists, and the evolutionary history data.