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Fig. 9.
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Temperature profile (red line) and density profile (dash-dotted black line) at the pre-SN stage as a function of the mass coordinate of a non-rotating stellar progenitor with MZAMS = 80 M⊙ and [Fe/H] = −2. A zoom-in on the innermost region of the core, up to 5 M⊙, is highlighted in the lower right box.
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