Online Material
![\begin{figure}
\par\includegraphics[width=16.8cm,clip]{13038f1.ps}\end{figure}](/articles/aa/olm/2009/46/aa13038-09/img42.png)
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Figure 1: Abundance ratios as a function of iron abundance for full sample of 64 stars. Dotted lines denote solar values. |
| Open with DEXTER | |
Table 1:
Derived stellar parameters, average abundance ratios [X/Fe] of volatile elements (
K), and slope of the [X/Fe] vs. 
relation for refractory elements (
K). Errors in
![${\rm [Fe/H]}$](/articles/aa/olm/2009/46/aa13038-09/img5.png){kind=small}
correspond to the 1-
scatter of the line-by-line abundances.
Table 2:
Abundance ratios [X/Fe] for C, O, Na, Al, Si, and S. Errors correspond to the 1-scatter
of the line-by-line abundances. A conservative value of 0.050 for the
error was assumed when only one line was available.
Table 3:
Abundance ratios [X/Fe] for Ca, Sc, Ti, V, Cr, and Mn. Errors correspond to the 1-
scatter of the line-by-line abundances. A conservative value of 0.050
for the error was assumed when only one line was available.
Table 4:
Abundance ratios [X/Fe] for Ni, Cu, Zn, Y, Zr, and Ba. Errors correspond to the 1-
scatter of the line-by-line abundances. A conservative value of 0.050
for the error was assumed when only one line was available.