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Fig. 8
Luminosity of solar-metallicity M dwarfs and substellar objects against time after formation according to Baraffe et al. (2003). The black dot marks HN Peg B and the orange dot shows CFBDS 1118. The luminosity of HN Peg B is log L/L⊙ = −4.76, with an error bar of 0.02 (Leggett et al. 2008), lower than the symbol size.
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