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

Open Access

Fig. 4

Condensate composition as a function of the radial position of silicon-bearing (left column) and iron-bearing (right column) minerals for a nebular composition consistent with the photosphere of HIP 43393. As in Fig. 3, the top and bottom rows denote the local initial conditions and nonlocal compositions after 100 kyr, respectively.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.