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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 3.

Pressure–temperature profiles of planets around G2, F0, and A0 host stars, corresponding to Teff = 5700 K, 7200 K, and 10,500 K, respectively. The figure at left shows a Jovian planet with Teq = 2250 K and the right figure shows a Jovian planet with Teq = 3000 K, with and without TiO and VO.

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