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Fig. 16

image

Bolometric luminosity (top) and effective temperature (bottom) as a function of the age of HD 19467B (gray area) compared to evolutionary tracks from the models COND (Baraffe et al. 2003), Saumon & Marley (2008) (for two treatments of the clouds), and Burrows et al. (1997) assuming the mass for the companion estimated from the orbital fit and the theoretical hydrogen-burning mass limit (data points). Small horizontal offsets are applied to all models except for COND for clarity.

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