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Showing content from https://link.springer.com/article/10.12942/lrr-2014-3/figures/15 below:

Figure 15 | The Evolution of Compact Binary Star Systems

The accumulation efficiency of helium as a function of the accretion rate for CO WD models of 0.6, 0.7, 0.81, 0.92, 1.02 M_⊙ (top to bottom), as calculated by Piersanti et al. (in prep.). Dotted and dashed lines represent the accumulation efficiency for CO WDs with initial masses 0.9 and 1.0 M_⊙, respectively, after Kato & Hachisu [347].

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