Fig. 7.

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Depletion factors as a function of gas density for the G10LG simulation at 400 Myr (black diamonds with standard deviation) compared to the results from Jenkins (2009; black dashed lines) and from De Cia et al. (2016; red dashed lines). The solid lines are the rescaled observational fits following Zhukovska et al. (2016). The purple and orange diamonds are the depletion factors for the G10LG simulation using a pyroxene compound (MgFeSi2O6), and an iron-poor olivine compound (Mg1.5Fe0.5SiO4), respectively, instead of the default olivine compound (MgFeSiO4) for silicates. The blue diamonds stand for the G10LG simulation without CO formation. For C depletion, we also show the data points from Jenkins (2009; triangles) and Parvathi et al. (2012; squares).
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