Image Details
Theoretical Transmission Spectra of Exoplanet Atmospheres with Hydrocarbon Haze: Effect of Creation, Growth, and Settling of Haze Particles. II. Dependence on UV Irradiation Intensity, Metallicity, C/O Ratio, Eddy Diffusion Coefficient, and Temperature
2019 The Astrophysical Journal 877 109.
Caption: Figure 2.
Temperature–pressure profiles of the atmosphere that we use to explore the dependence on temperature in Section 3.6. The green line represents the fiducial profile, which is calculated by the use of the analytical formula of Guillot (2010). Also shown is the profile for the irradiation temperature Tirr higher by 500 K than the fiducial value of 790 K, that is, 1290 K (red line), with the other parameters unchanged from the fiducial values.
© 2019. The American Astronomical Society. All rights reserved.