Free Access
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

Table A.1

Fe i and Fe ii lines used in the analysis.

thumbnail 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

Table A.2

Chemical elements (except Fe) and spectral lines in the analysis.


© ESO, 2011

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