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Fig. 6.
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Effective temperature and surface luminosity (upper and bottom panels) versus the cooling times for our 1.29, 1.31, 1.33, 1.35, and 1.369 M⊙ white dwarf sequences. Solid (dashed) lines correspond to the general relativity (Newtonian) cases. Cooling time is counted from the time of white dwarf formation.
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