Fig. 7
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Updated X-ray-to-bolometric ratio and Rossby numbers. Our results are in blue and those from Brown et al. (2022) in gray. They are compared with the Wright et al. (2018) model. Wright et al. (2018) saturation level appears excessively high for low-mass M stars, whereas Magaudda et al. (2022) reported a value close to −3.5 (see their Fig. 9).
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