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Stochasticity in Stellar Yields Reflected in Supernova Dust Masses Across All Massive-Star Progenitors
Massive stars, ending their lives as supernovae (SNe), are among the primary sources of dust in galaxies. In this study, we derive theoretical upper limits on dust masses as a function of SN progenitors, assuming non-rotating single stars of solar metallicity, with initial masses between 9 and 120 M
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