| Issue |
A&A
Volume 572, December 2014
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201424157e | |
| Published online | 28 November 2014 | |
Hot super-Earths and giant planet cores from different migration histories Corrigendum
1
Univ. Bordeaux, Laboratoire d’Astrophysique de Bordeaux, UMR
5804,
33270
Floirac,
France
e-mail:
christophe.cossou@u-bordeaux1.fr
2
CNRS, Laboratoire d’Astrophysique de Bordeaux, UMR
5804, 33270
Floirac,
France
e-mail:
rayray.sean@gmail.com
Key words: planets and satellites: formation / protoplanetary disks / planet-disk interactions / methods: numerical / errata, addenda
An error occurred during the production process. An incorrect Fig. 14 was published. The correct Fig. 14 is published below.
 |
Fig. 14 Comparison between the planets that formed in simulations with dissipating disks and observed extra-solar planets. Both samples are limited to the range R> 1.5 R⊕ (3.3 M⊕ assuming Earth density) and p< 200days. |
© ESO, 2014
All Figures
|
Fig. 14 Comparison between the planets that formed in simulations with dissipating disks and observed extra-solar planets. Both samples are limited to the range R> 1.5 R⊕ (3.3 M⊕ assuming Earth density) and p< 200days. |
| In the text | |
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