Fig. 1.
Abundance by mass of 4He, 12C, 16O, and 20Ne versus the outer ass coordinate for the 1.156 M⊙ DB WD models resulting from the evolutionary scenarios we studied. From top to bottom: ONe WD model from Camisassa et al. (2019), CO WD model resulting from reduced mass loss during progenitor evolution, and CO WD model implied by rotation.
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