Figure 5 from HELIOS: AN OPEN-SOURCE, GPU-ACCELERATED RADIATIVE TRANSFER CODE FOR SELF-CONSISTENT EXOPLANETARY ATMOSPHERES

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HELIOS: AN OPEN-SOURCE, GPU-ACCELERATED RADIATIVE TRANSFER CODE FOR SELF-CONSISTENT EXOPLANETARY ATMOSPHERES

Authors: Matej Malik, Luc Grosheintz, João M. Mendonça, Simon L. Grimm, Baptiste Lavie, Daniel Kitzmann, Shang-Min Tsai, Adam Burrows, Laura Kreidberg, Megan Bedell, Jacob L. Bean, Kevin B. Stevenson, and Kevin Heng

2017 The Astronomical Journal 153 56.

Provider: AAS Journals

Caption: Figure 5.

Elucidating the temperature dependence of the volume mixing ratios of the molecules used in the current study. For illustration, we set P = 1 bar and explore C/O = 0.1 (top panel), C/O = 0.5 (middle panel), and C/O = 1 (bottom panel). Within each panel, we explore the effects of varying the metallicity by ﹩1/3\times ﹩ and ﹩3\times ﹩ the solar value.

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