| Issue |
A&A
Volume 528, April 2011
|
|
|---|---|---|
| Article Number | A85 | |
| Number of page(s) | 11 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/201015138 | |
| Published online | 04 March 2011 | |
Online material
Appendix A: Chemical elements
Fe i and Fe ii lines used in the analysis.
 |
Fig. A.1
Upper panel: comparison of equivalent widths of M67-1194 and the FLAMES/UVES sky spectrum representing the Sun. 1D polynomial fits for both Fe i and Fe ii are shown as solid and dashed lines, respectively. Lower panel: the percentage equivalent-width difference of Fe i and Fe ii lines between M67-1194 and the FLAMES/UVES sky spectrum representing the Sun. Note that the abundances are not derived from equivalent widths, but from fits of synthetic spectra. |
| Open with DEXTER | |
Chemical elements (except Fe) and spectral lines in the analysis.
© ESO, 2011
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