Fig. 2.
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Nucleosynthesis of sub-Chandrasekhar-mass bare CO models with MWD = 1.06 M⊙ and Z = 0.035 with different distributions of 22Ne. The abundance of each isotope is given with reference to 56Fe and normalized to Solar System abundances: 
, where X stands for mass fraction. All the unstable species have been allowed to decay to their stable isobars.
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