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Fig. 1

image

Logarithm of the total mass of H (in solar masses) at the point of maximum effective temperature of the cooling sequence versus the white dwarf mass for Z = 0.0001,0.0005, and 0.001. In addition, we show the predictions of Renedo et al. (2010) for Z = 0.001 and Z = 0.01 progenitors.

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