Figure 7 from The Influence of Host Star Spectral Type on Ultra-hot Jupiter Atmospheres

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The Influence of Host Star Spectral Type on Ultra-hot Jupiter Atmospheres

Authors: Joshua D. Lothringer, and Travis Barman

2019 The Astrophysical Journal 876 69.

Provider: AAS Journals

Caption: Figure 7.

Mole fraction of different species in two ultra-hot Jupiters. The solid line is the T_eq = 3000 K planet irradiated by a G2 star (T_eff = 5700 K). The dashed line is the T_eq = 3000 K planet irradiated by an A0 star (T_eff = 10,500 K star).

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