All Figures

$\begin{figure} \par\includegraphics{9398_f1.eps} \end{figure}$ Figure 1: Observed Phoenix spectra of selected bulge giants as well as thick (Arcturus = HD 124897) and thin (HD 211075) disk stars.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{9398_f2.ps} \end{figure}$ Figure 2: The derived [O/Fe] ratios, as a function of [Fe/H], for the bulge (red triangles), thick disk (blue solid circles), thin disk (open green circles) and halo giants (stars). A typical error bar is shown. Note the similarities between the bulge and thick disk trends for $[{\rm Fe/H}] < -0.2$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm]{9398_f3.ps} \end{figure}$ Figure 3: The derived [C + N/Fe] ratios as a function of [Fe/H] for the bulge (red triangles), thick disk (blue solid circles), thin disk (open green circles) and halo giants (stars). A typical error bar is shown.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics{9398_f1.eps} \end{figure}$	Figure 1: Observed Phoenix spectra of selected bulge giants as well as thick (Arcturus = HD 124897) and thin (HD 211075) disk stars.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm]{9398_f2.ps} \end{figure}$	Figure 2: The derived [O/Fe] ratios, as a function of [Fe/H], for the bulge (red triangles), thick disk (blue solid circles), thin disk (open green circles) and halo giants (stars). A typical error bar is shown. Note the similarities between the bulge and thick disk trends for $[{\rm Fe/H}] < -0.2$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm]{9398_f3.ps} \end{figure}$	Figure 3: The derived [C + N/Fe] ratios as a function of [Fe/H] for the bulge (red triangles), thick disk (blue solid circles), thin disk (open green circles) and halo giants (stars). A typical error bar is shown.
Open with DEXTER