| Issue |
A&A
Volume 706, February 2026
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Planets, planetary systems, and small bodies | |
| DOI | https://doi.org/10.1051/0004-6361/202658886e | |
| Published online | 12 February 2026 | |
Pebble-driven migration of low-mass planets in the 2D regime of pebble accretion (Corrigendum)
1
Charles University, Faculty of Mathematics and Physics, Astronomical Institute,
V Holešovičkách 747/2,
180 00
Prague 8,
Czech Republic
2
Instituto de Ciencias Físicas, Universidad Nacional Autonoma de México, Av. Universidad s/n,
62210
Cuernavaca, Mor.,
Mexico
3
IRAP, Université de Toulouse, CNRS, UPS,
31400
Toulouse,
France
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
This article has no abstract.
Key words: hydrodynamics / methods: numerical / planets and satellites: formation / protoplanetary disks / planet-disk interactions / errata, addenda
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model. This email address is being protected from spambots. You need JavaScript enabled to view it. to support open access publication.
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.