$\begin{figure} \resizebox{8.8cm}{!}{\includegraphics{6249fig1.eps}}\end{figure}$ Figure 1: The distribution of chemical elements in the sampled stars (RX Vir is excluded, see explanation in the text). AB Leo - circles, CK Vir - squares, SV UMa - crosses, TY Vir - triangles. The vertical bars show the approximate abundance variations amongst the halo stars with [Fe/H] = -1.85.
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In the text

$\begin{figure} \resizebox{8.8cm}{!}{\includegraphics{6249fig1.eps}}\end{figure}$	Figure 1: The distribution of chemical elements in the sampled stars (RX Vir is excluded, see explanation in the text). AB Leo - circles, CK Vir - squares, SV UMa - crosses, TY Vir - triangles. The vertical bars show the approximate abundance variations amongst the halo stars with [Fe/H] = -1.85.
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$\begin{figure} \resizebox{8.8cm}{!}{\includegraphics{6249fig2.eps}}\end{figure}$	Figure 2: Mn I line profile fitting.
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