Fig. C.1
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Cumulative fraction of the contribution of different types of stars to 16O, 20Ne, and 36Ar (the most abundant stable isotopes of each element) enrichment as a function of 12+log(O/H) predicted by the chemical evolution model of Medina-Amayo (2023). Cyan line: asymptotic giant branch stars (AGBs); dark red line: type Ia supernovae (SNe Ia); magenta line: core collapse supernovae (CCSNe).
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