Evolving massive stars to core collapse with GENEC: Extension of equation of state, opacities and effective nuclear network

Open Access

Fig. 10.

Chemical structure for the pre-supernova models. Shown are the species ⁴He, ¹²C, ¹⁶O, ²⁰Ne, ²⁸Si, ³²S, ⁵⁴Fe, ⁵⁶Fe, ⁵⁶Co and ⁵⁶Cr as a function of enclosed mass. We also highlight the convective regions with the light blue hashed regions.

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