| Issue |
A&A
Volume 623, March 2019
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 2 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201833435e | |
| Published online | 25 February 2019 | |
The “memory” of the Oort cloud (Corrigendum)
1
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
e-mail: marc.fouchard@univ-lille1.fr
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
The q axes of Figs. 1 and 3 are oriented downward, whereas they should be oriented upward. The figures themselves are correct, only the orientation of the axes is wrong.
© ESO 2019
All Figures
 |
Fig. 1 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 | |
 |
Fig. 3 As Fig. 1 but for the D0 proto-Oort cloud. |
| Open with DEXTER | |
| In the text | |
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