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Fig. 2

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Atmospheric abundance profiles of the most important species computed by Cloudy employing the composite TP profile. Top: density relative to the total density of hydrogen for neutral hydrogen (HI; black solid), protons (HII; red), molecular hydrogen (H2; dark green), H (blue), H (violet), H (orange), and electrons (e; black dashed). Middle: Mixing ratios for hydrogen (black), H2 (black dotted), He (red), C (blue), O (dark green), Na (violet), K (orange), and electrons (bright green) asa function of atmospheric pressure. Neutral (XI), singly ionised (XII), and doubly ionised (XIII) species are shown as solid, dashed, and dash-dotted lines, respectively. Bottom: same as middle panel, but for Mg (red), Si (blue), Ca (dark green), and Fe (violet). The hydrogen, H2, and e mixing ratios are shown in both middle and bottom panels for reference.

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