Fraction of the initial mass of the star ejected by stellar winds during the whole stellar lifetime (red shaded area). The mass in the H-rich envelope, He-rich region, and CO core in the pre-supernova model as a function of the initial mass are indicated as black, white, and blue regions. Cases for various mass-loss rates during the RSG phase without and with rotation are shown. The symbols in the upper part of each panel indicate the range of effective temperatures of the model at the pre-supernova stage: log T_eff lower than 3.65 is indicated by (red) stars, log T_eff between 3.65 and 4.30 by (black) triangles, and log T_eff greater than 4.3 by (blue) circles.