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Fig. 12

image

Comparison between the numerical solutions (dashed lines) and the analytical solutions of model D (using the functional form of the coefficients given in Table 1) over a wide range of irradiation temperatures for a giant planet of solar composition orbiting a sun-like star. Here we used g = 25 m/s2, Tint = 100 K, and . Thick and thin lines represent convective and radiative zones, respectively.

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