Fig. 17
Comparison of TOI-1266 b & c with evaporation models. The coloured dots show the position in the plane of semi-major axis versus radius of simulated planets evolving under the effect of cooling, contraction, and atmospheric escape around a 0.5 M⊙ star at an age of 10 Gyr. One sees the radius valley and the sub-Neptunian desert. The colours show the planet mass. Black symbols show TOI-1266 b & c.
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