Fig. 14

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Positions of the investigated SSSs in the Teff-log g plane. Model dependencies for various WD masses (Nomoto et al. 2007) are shown by black dashed curves with indicated WD masses (in solar masses). The boundaries of the stable thermonuclear burning band are shown by the solid (upper boundary) and the dashed (lower boundary) red lines. The Eddington limit for solar H/He abundances is shown by the blue dashed line.
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