Figure 9 from Updated Spitzer Emission Spectroscopy of Bright Transiting Hot Jupiter HD 189733b

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Updated Spitzer Emission Spectroscopy of Bright Transiting Hot Jupiter HD 189733b

Authors: Kamen O. Todorov, Drake Deming, Adam Burrows, and Carl J. Grillmair

Todorov et al. 2014 The Astrophysical Journal 796 100.

Provider: AAS Journals

Caption: Figure 9.

Calculated temperature as a function of optical depth (upper panel) and pressure (lower panel), assuming a gray atmosphere with adopted Rosseland mean opacities from Freedman et al. (2008). The dashed line indicates the effective temperature of the planet, T_eff, at τ = 2/3.

Other Images in This Article

Copyright and Terms & Conditions