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Fig. 8


Unstable mode periods (Π) for = 1 in terms of the effective temperature, corresponding to the pre-WD model sequences with stellar masses M/M = 0.1554,0.1612,0.1650,0.1706,0.1763,0.1822,0.1868,0.1921, and 0.2026. Color coding indicates the value of the logarithm of the e-folding time (τe) of each unstable mode (right scale).

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