Fig. 13.
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Nucleosynthesis of sub-Chandrasekhar-mass bare CO detonation models with MWD = 1.06 M⊙ and Z = 0.038, either with uniform chemical composition through the WD or chemically stratified after migration of 56Fe and 22Ne to the center of the WD. The abundance of each isotope is given with reference to the final yield of 56Fe and normalized to Solar System abundances, as in Fig. 2.
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