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Fig. 4.

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H/H2O index strengths of XSL stars as a function of their (I − K) colours. Points are colour-coded by their effective temperatures from Arentsen et al. (2019), saturated at 10 000 K. Carbon stars are marked with circles. Supergiants are marked with diamonds. Both C-rich TP-AGB stars and supergiants are excluded from the division into static and variable stars. M dwarfs have weak H/H2O index strengths but can have red (I − K) colours, and they have been marked with triangles.

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