$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3607fig1.ps} \end{figure}$ Figure 1: Li equivalent widths vs. [Na/Fe] for the NGC 6752 stars. The typical measurement error bar is given in the left bottom corner.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3607fig2.ps} \end{figure}$ Figure 2: Li abundances vs. [Na/Fe] for the sample stars. For the sake of completeness, abundance values for both temperature scales are plotted: filled triangles G01 scale; filled (red) squares: Alonso scale.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3607fig3.eps} \end{figure}$ Figure 3: Li abundances vs. [O/Fe] and vs. [N/Fe] for the sample stars. [O/Fe] and [N/Fe] values are from Table 1 of Carretta et al. (2005), who used the G01 temperature scale.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3607fig1.ps} \end{figure}$	Figure 1: Li equivalent widths vs. [Na/Fe] for the NGC 6752 stars. The typical measurement error bar is given in the left bottom corner.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3607fig2.ps} \end{figure}$	Figure 2: Li abundances vs. [Na/Fe] for the sample stars. For the sake of completeness, abundance values for both temperature scales are plotted: filled triangles G01 scale; filled (red) squares: Alonso scale.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3607fig3.eps} \end{figure}$	Figure 3: Li abundances vs. [O/Fe] and vs. [N/Fe] for the sample stars. [O/Fe] and [N/Fe] values are from Table 1 of Carretta et al. (2005), who used the G01 temperature scale.
Open with DEXTER