The effects of transport processes on the bulk composition of the first generation of planetesimals interior to the water ice line

Open Access

Fig. 8

Comparison of the nonlocal and local radial behavior of elemental atomic percentages, n_i (in at.%) for elemental species i. The left and right panels show this comparison for the solar and HIP 43393 composition, respectively. Since we focus on the disk inside ~1.5 au, the minerals do not contain notable amounts of C or N.

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