Image Details

Choose export citation 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 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.

Other Images in This Article

Show More

Copyright and Terms & Conditions