| Issue |
A&A
Volume 601, May 2017
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201527385e | |
| Published online | 17 May 2017 | |
The origin and evolution of r- and s-process elements in the Milky Way stellar disk (Corrigendum)
1 Lund Observatory, Department of Astronomy and Theoretical Physics, Box 43, 221 00 Lund, Sweden
e-mail: cbattistini@lsw.uni-heidelberg.de
2 Current address: Zentrum für Astronomie der Universität Heidelberg, Landessternwarte, Königstuhl 12, 69117 Heidelberg, Germany
Key words: stars: abundances / stars: solar-type / Galaxy: disk / Galaxy: evolution / solar neighborhood / errata, addenda
An error occurred during the production process. Figure 3 published in the original article was wrong. The correct figure is presented here.
 |
Fig. 3
[Eu/Ba] as a function of [Fe/H]. The full sample is divided into thin and thick disks according to our age-selection criterion. The dotted line represents a pure r-process ratio derived from Bisterzo et al. (2014). The average error is also presented. |
© ESO, 2017
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.