[https://doi.org/10.1051/0004-6361/202039640]
[https://doi.org/10.1051/0004-6361/202141096]
| Issue |
A&A
Volume 659, March 2022
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 3 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/202141096e | |
| Published online | 11 March 2022 | |
How drifting and evaporating pebbles shape giant planets (Corrigendum)
1
Max-Planck-Institut für Astronomie,
Königstuhl 17,
69117
Heidelberg,
Germany
2
Centre for ExoLife Sciences, Niels Bohr Institute,
Øster Voldgade 5,
1350
Copenhagen,
Denmark
e-mail: aaron.schneider@nbi.ku.dk
3
Instituut voor Sterrenkunde,
KU Leuven, Celestijnenlaan 200D,
3001
Leuven,
Belgium
This article has no abstract.
Key words: accretion, accretion disks / planets and satellites: formation / protoplanetary disks / planet-disk interactions / errata, addenda
© A. D. Schneider and B. Bitsch 2022
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.
Open Access funding provided by Max Planck Society.
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