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Core-Collapse Supernovae from Single and Binary-Stripped Massive Stars - I. Explodability and Nucleosynthesis
Binary interaction can substantially alter massive-star evolution and pre-supernova structure, changing core-collapse outcomes and nucleosynthetic yields. We compare explodability and nucleosynthesis in 66 non-rotating, solar-metallicity single-star and binary-stripped progenitors spanning zero-age
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