摘要：After publication of Breslau et al. (2017) we noticed a mis-
take in the plot script used to produce Figs. 2d, 3d, and 5d.
These images should have shown the final semi-major axes of
the bound particles relative to the radii of their initial orbits de-
pending on their virtual pericentre positions (VPPs). Due to an
incorrect multiplication with (1 − e), the images instead showed
the final periapsides of the bound particles relative to their initial
orbital radii. In this erratum we present the corrected images (see
Fig. 1).
关键词：enmethods: numericalprotoplanetary disksgravitationplanets and satellites: dynamical evolution and stabilityscatteringerrata, addenda
