Figure 10 from 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

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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

Authors: Yui Kawashima, and Masahiro Ikoma

2019 The Astrophysical Journal 877 109.

Provider: AAS Journals

Caption: Figure 10.

Same as Figure 3 but for the cases of (a) and (b) 10 × solar, (c) and (d) 100 × solar, and (e) and (f) 1000 × solar metallicity atmospheres.

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