Figure 16 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 16.

Same as Figure 3, but for two different values of the eddy diffusion coefficient, K_zz: (a) and (b) K_zz = 1 × 10⁹ cm² s⁻¹; (c) and (d) K_zz = 1 × 10⁵ cm² s⁻¹.

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