| 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 | |
Grain size segregation in debris discs (Corrigendum)
1 LESIA-Observatoire de Paris, CNRS, UPMC Univ. Paris 6, Univ. Paris-Diderot, France
e-mail: philippe.thebault@obspm.fr
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.
 |
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). |
© ESO, 2014
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