| Issue |
A&A
Volume 572, December 2014
|
|
|---|---|---|
| Article Number | A108 | |
| Number of page(s) | 21 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201424533 | |
| Published online | 04 December 2014 | |
Online material
Appendix A: Light element correlations
We here present plots of [X/Fe] vs. [Na/Fe] to trace elements that vary in step with the light element variations.
 |
Fig. A.1
[X/Fe] vs. [Na/Fe] from O to Ti. In each plot is shown representative uncertainties. Symbols the same as in Fig. 10. |
| Open with DEXTER | |
 |
Fig. A.2
[X/Fe] vs. [Na/Fe] from V to Zr. In each plot is shown representative uncertainties. Symbols the same as in Fig. 10. |
| Open with DEXTER | |
 |
Fig. A.3
[X/Fe] vs. [Na/Fe] from Mo to Dy. In each plot is shown representative uncertainties. Symbols the same as in Fig. 10. |
| Open with DEXTER | |
© ESO, 2014
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