Fig. 6
Comparison of the equal-mass binary HZ to acrit. The curves correspond to different choices of the binary’s orbital eccentricity, up to 0.5, as shown in the legend. The blue shaded region is the HZ from Kopparapu et al. (2013), but with the stellar luminosity doubled to account for the two stars. The approximate runtime was 15 s. github.com: cbp_dynamic_stability/HZ_CBP/
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