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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.
- Provider: AAS Journals
Caption: Figure 18.
Transmission spectrum models for the atmospheres with haze for the cases of Tirr = 1290 K (thick red line) and Tirr = 790 K (thick green line; same as the green line in Figure 5). The transmission spectrum for the atmosphere without haze for the cases of Tirr = 1290 K (red thin line) and Tirr = 790 K (thin green line; same as the black line in Figure 5) are also plotted. Note that the transmission spectrum models are smoothed for clarity.
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