Fig. 3.
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Energy production rates ϵ [erg.g−1.s−1] inside a 15 M⊙ rotating star for varying reaction rates. Left: Energy during shell C-burning, approximatively 3000 years after core C-ignition. Right: Energy during core O-burning at central X16O = 0.3. The pale areas in orange indicate where the gravitational energy is negative, i.e. corresponding to an expansion.
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