Volume 528, April 2011
|Number of page(s)||11|
|Published online||04 March 2011|
Fe i and Fe ii lines used in the analysis.
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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