Grain size segregation in debris discs (Corrigendum)
1 LESIA-Observatoire de Paris, CNRS, UPMC Univ. Paris 6, Univ. Paris-Diderot, France
2 Université Joseph Fourier/CNRS, LAOG, UMR 5571 Grenoble, France
Key words: planet-disk interactions / planets and satellites: formation / circumstellar matter / errata, addenda
An error occurred during the production process. An incorrect Fig. 10c was published. The correct Fig. 10 is published below.
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