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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 5.

Relative contribution of different opacity sources to the absorption mean opacity, κJ, at different pressures in the atmosphere for the Teq = 2250 K temperature structure without TiO/VO (left) and the Teq = 3000 K structure with TiO/VO (right), both irradiated by an A0-type star. TiO opacity is included in the left figure to show the contribution TiO would have if it were included.

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