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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. 7.—

Fig. 7.—

Dominant stability regimes in chemical equilibrium at 100 mbar for gas-phase carbon species as a function of temperature and bulk C/O ratio for 300× solar metallicity (left) and as a function of temperature and metallicity for a solar C/O ratio (right). Conditions where graphite is stable are shaded. A color version of this figure is available in the online journal.