Non-standard s-process in massive rotating stars - Yields of 10–150 M⊙ models at Z = 10−3

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Fig. 8.

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Internal Ω profile, D_shear coefficient, and other diffusion coefficients in Eq. (2) for the rotating 25 (left panel) and 150 M_⊙ models (right panel) during the core He-burning phase (Y_c = 0.66). Grey areas represent the convective zones and the dashed lines show the K/D_h ratio.

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