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. Author manuscript; available in PMC: 2019 Mar 4.
Published in final edited form as: Astrophys J. 2013 Oct 11;777(1):34. doi: 10.1088/0004-637X/777/1/34

Fig. 6.—

Fig. 6.—

Equilibrium mole fractions for different gas-phase species as a function of temperature and C/O ratio for a 100-mbar pressure and a metallicity X/H = 300× solar (where X represents all elements except H, He, Ne, and O, with the O abundance being defined through the C/O ratio).