Fig. 15
Bolometric luminosity of HD 19467B computed using the NIRC2 photometry in the Ks band (left) and in the J band (right) and the relations of Filippazzo et al. (2015) for field dwarfs as a function of the mass estimated from the orbital fit and the theoretical hydrogen-burning mass limit (see text). For comparison, the model isochrones of Baraffe et al. (2003) are indicated.
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