All Figures

$\begin{figure} \par\includegraphics[width=12.5cm,clip]{fig1.eps} \end{figure}$ Figure 1: Observed a versus (g₁-y) and V versus (g₁-y)diagrams for our programme clusters. The solid line is the normality line whereas the dotted lines are the confidence intervals corresponding to 99.9% ( left panels). The error bars for each individual object are the mean errors. The detected peculiar objects are marked with asterisks. Only members (filled circles) have been used to derive the normality lines. The fitting parameters are listed in Table 4. The isochrones (right panels) were taken from Claret et al. (2003) and Claret (2004) and are based on the $\Delta a$ photometric system. The derived ages, reddening and distance moduli are given in Table 2.
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In the text

$\begin{figure} \par\includegraphics[width=12.35cm,clip]{fig2.eps} \end{figure}$ Figure 2: Observed a versus (g₁-y) and V versus (g₁-y)diagrams for our programme clusters. The symbols are the same as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{fig3.eps} \end{figure}$ Figure 3: Observed a versus (g₁-y) and V versus (g₁-y)diagrams for our programme clusters. The symbols are the same as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=12.35cm,clip]{fig2.eps} \end{figure}$	Figure 2: Observed a versus (g₁-y) and V versus (g₁-y)diagrams for our programme clusters. The symbols are the same as in Fig. 1.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=12cm,clip]{fig3.eps} \end{figure}$	Figure 3: Observed a versus (g₁-y) and V versus (g₁-y)diagrams for our programme clusters. The symbols are the same as in Fig. 1.
Open with DEXTER