Fig. 2
Post-RLO evolution of surface gravity versus effective temperature for a ~ 0.23 M⊙ proto-WD produced from an LMXB donor star with Z = 0.01. Three different models are shown: basic configuration (top panel), diffusion configuration (middle panel) and diffusion+rotation configuration (bottom panel). Note that the computations are stopped when the age of the model star reaches 14 Gyr (since ZAMS).
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