Free Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201731582]


Issue
A&A
Volume 650, June 2021
Article Number C1
Number of page(s) 2
Section Stellar atmospheres
DOI https://doi.org/10.1051/0004-6361/201731582e
Published online 08 June 2021

In Figs. 1 and 2, we present the corrected versions of Figs. 5 and 6 from Mashonkina et al. (2017). Compared with the original paper, the changes only concern including the X-axis in the bottom panels of the figures.

References

  1. Mashonkina, L., Jablonka, P., Sitnova, T., Pakhomov, Y., & North, P. 2017, A&A, 608, A89 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

© ESO 2021

All Figures

thumbnail Fig. 1

Stellar [Na/Mg] and [Al/Mg] LTE (left column) and NLTE (right column) abundance ratios in Sculptor (red circles), Ursa Minor (green circles), Sextans (squares), Fornax (rhombi), Boötes I (triangles), UMa II (inverted triangles), and Leo IV (five-pointed star) dSphs and the MW halo (black circles). The NLTE ratio [Na/Mg] = 0.68 for Sex 24–72 is not shown.

Open with DEXTER
In the text
thumbnail Fig. 2

Left column: [Sr/Fe] and [Ba/Fe] NLTE abundance ratios as a function of metallicity for our sample stars. Right column: [Sr/Mg] and [Ba/Mg] NLTE abundance ratios as a function of Mg abundance. Symbols and colours are the same as in Fig. 1. Upper limits in the Ba and Sr abundances are indicated with arrows.

Open with DEXTER
In the text

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