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Fig. 9.

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Left panel: periods of excited  = 1 g modes as a function of the effective temperature, with the palette of colors (right scale) indicating the logarithm of the e-folding time (τe in years), for the DB WD sequence with M = 0.584 M. Right panel: same as left panel, but for  = 2 modes. In both panels, the pulsation periods of the DBV star GD 358, with the identification of according to our asteroseismological model (see Table 4), are shown as horizontal segments, where their widths represent the possible Teff interval, according to spectroscopy.

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