EDP Sciences
Free Access
Erratum
This article is an erratum for: [this article]

Issue
A&A
Volume 570, October 2014
Article Number C1
Number of page(s) 1
Section Planets and planetary systems
DOI https://doi.org/10.1051/0004-6361/201322052e
Published online 07 October 2014

An error occurred during the production process. An incorrect Fig. 10c was published. The correct Fig. 10 is published below.

thumbnail Fig. 1

Extended disc perturbed by an embedded planet. Azimuthally averaged radial distribution of the geometrical cross-section, as a function of particle sizes, for four different configurations: a) nominal (run G); b) Saturn-mass planet (μ = 2 × 10-4, run J); c) high optical depth (τ = 2 × 10-2, run I); d) low optical depth (τ = 5 × 10-5, run H).

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© ESO, 2014

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