Total masses of selected isotopes in the winds of the massive stars from the two sets of models adopted in this work. Solid curves are yields from HMM05 (with rotation) and dotted curves from LC06 (no rotation), in both cases interpolated between model results. The points correspond to results of the HMM05 models with no rotation and, in general, agree well with LC06 results except for the 60 M_⊙ star.