Volume 601, May 2017
|Number of page(s)||1|
|Section||Galactic structure, stellar clusters and populations|
|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
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.
[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.
|Open with DEXTER|
© ESO, 2017
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