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Fig. 1.
Upper panel: inner distribution of O, C, and He in terms of the outer mass fraction corresponding to the expectations from a typical DBV model of mass ∼0.58 M⊙ resulting from the complete progenitor evolution. Bottom panel: same as above, but for the asteroseismic model for the DBV KIC 08626021 of Giammichele et al. (2018).
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