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Fig. 5.

image

Bolometric luminosity vs. age of HD 72946B (gray area) compared to evolutionary tracks from the models COND (Baraffe et al. 2003), Saumon & Marley (2008; for two treatments of the clouds), Burrows et al. (1997), and Baraffe et al. (2015) assuming the mass range for the companion from the orbital fit (data points). Small horizontal offsets are applied to all models except for COND for clarity.

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