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Fig. 15

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List of binary systems where the stellar component hosting planets is a low-mass star with Teff < 4000 K. The systems are arranged according to the projected separation between the two stellar components of the binary, with TOI-2267 standing out as the closest binary system found to harbour planets. The sizes of the stars are to scale relative to each other, and their colours represent their stellar temperatures. Blue circles indicate transiting planets, which are also scaled relative to each other. In contrast, blue triangles denote non-transiting planets (detected by radial velocity only), all set to an arbitrary size. For each system, the orbital distances from the host star where the insolation flux ranges from 10 to 0.1 S are highlighted.

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