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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 9.

High-resolution (R ∼ 500,000) spectra of the Teq = 3000 K hot Jupiters, focusing on the first overtone band of CO at 2.3 μm. The figure on the right zooms in on the figure on the left.

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