Masses, revised radii, and a third planet candidate in the 'Inverted' planetary system around TOI-1266
Is the population of close-in planets orbiting M dwarfs sculpted by thermally driven escape or is it a direct outcome of the planet formation process? A number of recent empirical results strongly suggest the latter. However, the unique architecture of the TOI-1266 system presents a challenge to models of planet formation and atmospheric escape
Cloutier, Ryan et al.
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2024