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.
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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. |
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© ESO, 2017