The Influence of Host Star Spectral Type on Ultra-hot Jupiter Atmospheres
Authors: Joshua D. Lothringer, and Travis Barman
2019 The Astrophysical Journal87669.
Provider: AAS Journals
Caption: Figure 6.
The temperature structure of the Teq = 3000 K ultra-hot Jupiters with TiO from Figure 3 irradiated by blackbodies (dotted), LTE stellar spectra (dashed), and the NLTE stellar spectra (solid) shown in Figures 1 and 2.
