Volume 623, March 2019
|Number of page(s)||2|
|Section||Planets and planetary systems|
|Published online||25 February 2019|
The “memory” of the Oort cloud (Corrigendum)
LAL-IMCCE, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, Univ. Lille., 1 Impasse de l’Observatoire, 59000 Lille, France
2 RISE Project Office, National Astronomical Observatory of Japan, 2-12 Hoshigaoka-cho, Mizusawa, Iwate 023-0816, Japan
3 CfCA, NAOJ, Mitaka, Tokyo 181-8588, Japan
Key words: comets: general / Oort Cloud / errata, addenda
© ESO 2019
From top to bottom panels: distribution of comets in (a, q), (a, cos (iE), (a, ωG) and (a, ΩG) planes at four different epochs t = 250 Myr and 1, 2 and 4 Gyr. For visibility, the bin sizes are constant along any axis. However the density function is computed in number of comets per au for the perihelion distance and per au−1 for the semi-major axis. The data comes from the evolution of the I0 proto-Oort cloud.
|Open with DEXTER|
|In the text|
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