Stellar yields in M_⊙ (Eq. (3)) as a function of the initial mass M_ini for the non-rotating (dashed lines) and rotating (solid lines) models. The mass cut is set using the relation of Maeder (1992). Isotopes ⁸⁸Sr, ¹³⁸Ba, and ²⁰⁸Pb are shown. Green patterns between 15 and 40 M_⊙ are the yields of the F16 models. The small and big red arrows at M_ini = 25 M_⊙ indicate the yields of ¹³⁸Ba for the fast-rotating 25 M_⊙ model and the fast-rotating 25 M_⊙ models with a lower ¹⁷O(α, γ) rate respectively. The same arrows are plotted for ⁸⁸Sr and ²⁰⁸Pb. Arrows at M_ini = 120 M_⊙ represent the 120 M_⊙ model with a lower ¹⁷O(α, γ) rate. We note that some arrows are not visible because there are too small.