Fig. 5
Left: absolute value of the maximum rate of period change in terms of the stellar mass corresponding to ℓ = 1g modes with selected radial orders k, for WD models with effective temperatures in the range 8000 ≲ Teff ≲ 10 000 K. Middle: same as in the left panel, but for ℓ = 1p modes. Right: same as in the left panel, but for radial (ℓ = 0) modes.
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