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Fig. 13

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The mass as a function of Teff for substellar objects, according to evolutionary models of 10 Myr and 50 Myr objects (Chabrier et al. 2000). The range of effective temperatures for AB Pic B from the best fit models is shown with solid lines and the range previously reported (Bonnefoy et al. 2010) is shown with dashed lines for comparison. The age of AB Pic B is expected to be between 10 Myr and 50 Myr.

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