Rotating models of very massive close binary stars at solar metallicity: Evolution and remnant masses
To investigate the evolution of massive close binary systems at solar metallicity, we utilized the Modules for Experiments in Stellar Astrophysics (MESA) numerical code to compute a grid of 2,880 detailed evolutionary models. These models consist of rotating stars with initial masses between 100 and 250 ̊m M_⊙ and init...