Fig. 4.
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Left: cooling curves for a 67 MJup (top) and a 53 MJup (bottom) BD, respectively, representative of the ϵ Ind Bab system. The solid line shows the present models based on the CD21 EOS; while the dashed line shows the Phillips et al. (2020) models based on the CMS19 EOS. Right: BD isochrones typical of the inferred age of the ϵ Ind Bab system, calculated with the present (red) and Phillips et al. (2020) (black) models.
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