The impact of chemical differentiation of white dwarfs on thermonuclear supernovae

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Fig. 5

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Chemical composition of the ejecta for the model with ρ_DDT function of the mass fractions of ¹²C and ²²Ne as given by Eq. (2) at the beginning of the cooling process: X(¹²C) = 0.36, X(²²Ne) = 0.020 (see Table 1).

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