Fig. 3.
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Main elements as function of mass coordinate for runaway 1000 s after the supernova for mass coordinates that remain bound after supernova explosion. Unlike in Bhat et al. (2025), 56Ni does not dominate the mass fraction at the surface of the runaway. 56Fe is present due to the primordial solar abundance assumed. 20Ne and 24Mg are elevated most likely due to carbon burning on the secondary.
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