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Thermal Structure and Radius Evolution of Irradiated Gas Giant Planets

  • Authors: Phil Arras and Lars Bildsten

Arras & Bildsten 2006 The Astrophysical Journal 650 394.

  • Provider: AAS Journals

Caption: Fig. 21.

Equilibrium temperature vs. ﹩T_{\mathrm{deep}\,}﹩. The temperature of the deep isotherm ﹩T_{\mathrm{deep}\,}﹩ is expected to be strongly correlated with the equilibrium temperature ﹩T_{\mathrm{eq}\,}﹩, giving a line sloping up to the right. Bracketed lines give constraints on ﹩T_{\mathrm{deep}\,}﹩, while arrows pointing downward represent upper limits.

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