$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig1.eps}\end{figure}$ Figure 1: Location in the H-R diagram of nonactive (open circles) and active (black circles) stars studied in this work.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig2.eps}\end{figure}$ Figure 2: Errors on temperature, $\sigma$ $T_{\rm eff}$ , vs. $T_{\rm eff}$ . Notation is the same as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig3.eps}\end{figure}$ Figure 3: Errors on temperature, $\sigma$ $T_{\rm eff}$ , vs. V magnitudes. Notation is the same as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig6.eps}\end{figure}$ Figure 6: Trends in the studied elements with [Fe/H] of nonactive stars (open circles) and active (black circles) stars.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig7.eps}\end{figure}$ Figure 7: Trends in the studied elements with [Fe/H] of nonactive stars (open circles) and active (black circles) stars.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig8.eps}\end{figure}$ Figure 8: The dependence of Li abundance on the rotational velocity $v\sin i$ , the notation is the same as in Fig. 1. The stars with the upper limit of the Li abundance marked by an arrow.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig9.eps}\end{figure}$ Figure 9: Index of chromospheric activity GrandS with rotational velocity. The notation is the same as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0360fig10.eps}\end{figure}$ Figure 10: The dependence of Li abundance on index of chromospheric activity S, the notation is the same as in Fig. 8.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig1.eps}\end{figure}$	Figure 1: Location in the H-R diagram of nonactive (open circles) and active (black circles) stars studied in this work.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig2.eps}\end{figure}$	Figure 2: Errors on temperature, $\sigma$ $T_{\rm eff}$ , vs. $T_{\rm eff}$ . Notation is the same as in Fig. 1.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig3.eps}\end{figure}$	Figure 3: Errors on temperature, $\sigma$ $T_{\rm eff}$ , vs. V magnitudes. Notation is the same as in Fig. 1.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig4.eps}\end{figure}$	Figure 4: Turbulent velocity $V_{\rm t}$ versus $T_{\rm eff}$ . Notation is the same as in Fig. 1.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig5.eps}\end{figure}$	Figure 5: Rotational velocity $v\sin i$ versus $T_{\rm eff}$ . Notation is the same as in Fig. 1.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig6.eps}\end{figure}$	Figure 6: Trends in the studied elements with [Fe/H] of nonactive stars (open circles) and active (black circles) stars.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig7.eps}\end{figure}$	Figure 7: Trends in the studied elements with [Fe/H] of nonactive stars (open circles) and active (black circles) stars.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig8.eps}\end{figure}$	Figure 8: The dependence of Li abundance on the rotational velocity $v\sin i$ , the notation is the same as in Fig. 1. The stars with the upper limit of the Li abundance marked by an arrow.
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$\begin{figure} \par\includegraphics[width=8.6cm,clip]{0360fig9.eps}\end{figure}$	Figure 9: Index of chromospheric activity GrandS with rotational velocity. The notation is the same as in Fig. 1.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0360fig10.eps}\end{figure}$	Figure 10: The dependence of Li abundance on index of chromospheric activity S, the notation is the same as in Fig. 8.
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