Figure 14 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

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 14.

Same as Figure 4 but for the cases of atmospheres with C/O = (a) 1, (b) 10, and (c) 1000.

Other Images in This Article

Copyright and Terms & Conditions