Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=12cm,clip]{3287fig1.eps} \end{figure}$ Figure 1: Observed a versus (g₁-y)diagrams for our programme clusters. The solid line is the normality line and the dotted lines are the confidence intervals corresponding to 99.9%. 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. For Stock 16, we also included the PMS objects (open circles) to show the apparent emission (location below the normality line) for these stars. The fitting parameters are listed inTable 3.
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In the text

$\begin{figure} \par\includegraphics[width=12.2cm,clip]{3287fig2.eps} \end{figure}$ Figure 2: Observed V versus (g₁-y)diagrams for our programme clusters. The isochrones are based on the $\Delta a$ photometric system and were taken from Claret et al. (2003). The derived ages, reddening, and distance moduli are listed in Table 2. The symbols are the same as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=12.2cm,clip]{3287fig2.eps} \end{figure}$	Figure 2: Observed V versus (g₁-y)diagrams for our programme clusters. The isochrones are based on the $\Delta a$ photometric system and were taken from Claret et al. (2003). The derived ages, reddening, and distance moduli are listed in Table 2. The symbols are the same as in Fig. 1.
Open with DEXTER