The impact of asteroseismically calibrated internal mixing on nucleosynthetic wind yields of massive stars

Open Access

Fig. 7.

Same as Fig. 5, but for ³⁶Cl (left) and ⁴¹Ca (right). The lower panels show the ratio between the yield of the reference models (log(D_env/cm² s⁻¹) = 0) and the models with the other values for log(D_env/cm² s⁻¹). Mind that unlike in Fig. 5, here the y-scale for the ratio is in log.

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