Fig. 8.
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Selected properties of the last computed structure in the rotating model. We report the abundance of 4He, 12C, and 16O in the upper panel (solid lines) and the ω and ωcr profiles in the lower panel (solid and dashed lines, respectively). For comparison, in the upper panel we report the abundances of the same isotopes in the initial 0.75 M⊙ WD model (dashed lines).
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