Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267

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Fig. 13

Polar plot of the apsidal trajectory (e_be_c vs Δω) for the TOI-2267 b and c planets over a period of 1 Myr. In this particular scenario, the planetary eccentricities were chosen as 0.025. The figure shows that the apsidal modes are librating around the 3:2 MMR (see Sect. 7.2).

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