Exploring deep and hot adiabats as a potential solution to the radius inflation problem in brown dwarfs - Long-timescale models of the deep atmospheres of KELT-1b, Kepler-13Ab, and SDSS1411B

Open Access

Fig. 5

1D models of sub-stellar ‘day-side’ (reds) and non-irradiated ‘night-side’ (blues) for the three brown dwarfs under consideration here: Profiles for Kepler-13Ab are plotted with solid lines, with dashed lines used for KELT-1b, and dotted lines for SDSS1411B.

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