Fig. 2.
Masses and radii of the ten very-low-mass stars. The Exeter/Lyon (E/L; Baraffe et al. 2015, 1998, 2003) 1 Gy (red) and 5 Gy (blue) isochrones are shown, for solar metallicity, [Fe/H] = 0.0 dex (solid lines), and sub-solar metallicity, [Fe/H] = −0.5 dex (dashed lines). The Dartmouth (DMTH; Dotter et al. 2008) (dashed, grey) and PARSEC (PSEC; Marigo et al. 2017) isochrones (dot-dashed, grey) are also shown; for sub-solar (smallest radii), solar, and super-solar ([Fe/H] = +0.5 dex) metallicity (largest radii).
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