Fig. 6
Age delays, in percentage with respect to the case in which phase separation is not considered, due to carbon-oxygen phase separation according to the phase diagram of Horowitz et al. (2010) and Segretain & Chabrier (1993), dashed and solid lines, respectively. Upper and bottom panel correspond to the 0.593 and 0.878 M⊙ white dwarf sequences, respectively.
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