Volume 572, December 2014
|Number of page(s)||1|
|Section||Planets and planetary systems|
|Published online||28 November 2014|
Hot super-Earths and giant planet cores from different migration histories Corrigendum
Univ. Bordeaux, Laboratoire d’Astrophysique de Bordeaux, UMR
2 CNRS, Laboratoire d’Astrophysique de Bordeaux, UMR 5804, 33270 Floirac, France
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.
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.
|Open with DEXTER|
© ESO, 2014
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