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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. 14.

Radius vs. age for ﹩M/ M_{\mathrm{J}\,}=0.32﹩, 1.0, and 3.2 and ﹩T_{\mathrm{deep}\,}=500﹩, 1500, 2500, and 3500 K, from bottom to top within each panel. Solid lines show the numerical evolution, while dashed lines show the fitting formula in eq. (32).

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