Enriching inner discs and giant planets with heavy elements

Open Access

Fig. 3

Time evolution integration of heavy-element content of the gas phase at 0.5 AU either from the solids (see Fig. 1) or the vapour (see Fig. 2) for discs with R_c = 250 AU and α = 10⁻⁴ (left) and α = 10⁻³ (right).

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