A discontinuity in the luminosity–mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202140536e]

Fig. 6.

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Luminosity–mass relation for metallicities Z = 0.0001 (top), Z = 0.001 (middle), and Z = 0.01 (bottom) at model ages 1, 3, 5, 7, and 9 Gyr. A movie of the full time lapse is available online for the Z = 0.001 model set.

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