Fig. 12
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Solar convective zone abundance changes created by accretion of a disk forming Jupiter as a function of disk viscosity α for ufrag = 1 m s−1 (blue) and ufrag = 10 m s−1 (orange). The data points show the mean value for simulations with R0 ∈ {75 AU, 150 AU} and M0 ∈ {0.05, 0.1}, and the error bars indicate the standard deviation.
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