Issue |
A&A
Volume 508, Number 1, December II 2009
|
|
---|---|---|
Page(s) | L17 - L20 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/200913038 | |
Published online | 12 November 2009 |
Online Material
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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
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.
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