Fig. 8.
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Ye distributions of the ejecta color-coded by the ZAMS mass of the progenitor star for each of the three sets of simulations. Notice that we separated the single and binary stars of F23 in the bottom two panels. Lower-mass stars reach higher Ye, as also seen in 3D simulations (Melson et al. 2015; Müller et al. 2019; Stockinger et al. 2020; Sandoval et al. 2021; Wang & Burrows 2024c).
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