Fig. 11.
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Same as Figure 7 but for the most central region of the progenitor with MZAMS = 80 M⊙ and [Fe/H] = −2, where we can better appreciate the fallback of the layers right after being accelerated by the shock wave. We show the behavior of the shell enclosing different values of mass, of 1 M⊙ (each solid light gray lines) and 5 M⊙ (each dotted purple line), respectively.
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