The effect of nonlocal disk processes on the volatile CHNOS budgets of planetesimal-forming material

Open Access

Fig. A.1

Number densities n_x of gas and ice phase molecules in the background disk model. The number densities are presented in units of log₁₀(molecules m⁻³). The white boxes indicate the monomer sampling region defined in Sect. 2.3, and the white dashed lines are abundance contours corresponding to the labels at the color bar.

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