Open Access

Fig. 1


Temperature profiles of a Jupiter size planet around three types of host stars (A0 – solid blue line, F0 – dashed green line, G2 – dotted red line, and K0 – dash-dotted brown line) calculated with HELIOS and grouped according to the equilibrium temperatures of 1000 K (left), 2000 K (middle), and 3000 K (right), respectively. The parameterized profile after Parmentier & Guillot (2014) with temperature inversion in upper atmospheric layers is shown with a full black line.

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