Stellar mass at the end of core hydrogen burning versus initial mass for our sequences with initial rotational velocities of v_rot,i ≃ 0 km s^-1, 300 km s^-1, and 500 km s^-1 (filled symbols). The open symbols correspond to the LMC models of Yusof et al. (2013) with and without rotation. The dotted straight line corresponds to the location where the stellar mass at the end of core hydrogen burning equals the initial mass, i.e. to negligible mass loss.