All Figures

$\begin{figure} \includegraphics[origin=rb,angle=-90,width=12cm,clip]{4157fig1.eps}\end{figure}$ Figure 1: Spectral energy distributions for 45 M 31 GCs and GC candidates.
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In the text

$\begin{figure} \par {\includegraphics[angle=-90,width=8.3cm,clip]{4157fig2.eps} } \end{figure}$ Figure 2: Graphs of the best-fit integrated colors of SSP models plotted on top of the intrinsic integrated colors for 14 GCs. Open circles with error bars represent the intrinsic integrated color of a GC, the thick line represents the best fit of the integrated color of a SSP model. The Y-axis is the ratio of the flux in each filter to the flux in filter BATC08.
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In the text

$\begin{figure} \par {\includegraphics[angle=-90,width=8.3cm,clip]{4157fig3.eps} } \par\end{figure}$ Figure 3: Contours of $\Delta \chi 2=2.30$ for a few M 31 globular clusters.
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In the text

$\begin{figure} \par {\includegraphics[angle=-90,width=8.3cm,clip]{4157fig4.eps} } \end{figure}$ Figure 4: Graphs of the best-fit integrated colors of SSP models plotted on top of the intrinsic integrated colors for 19 confirmed GCs. Open circles with error bars represent the intrinsic integrated color of an object, the thick line represents the best fit of the integrated color of a SSP model. The Y-axis is the ratio of the flux in each filter to the flux in filter BATC08.
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In the text

$\begin{figure} \par {\includegraphics[width=8.6cm,clip]{4157fig5.eps} } \end{figure}$ Figure 5: The location of the clusters ontop of M 31 image.
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In the text

$\begin{figure} \par {\includegraphics[angle=-90,width=8.8cm,clip]{4157fig6.eps} } \end{figure}$ Figure 6: Metallicity as a function of age for globular clusters of M 31.
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In the text

$\begin{figure} \includegraphics[origin=rb,angle=-90,width=12cm,clip]{4157fig1.eps}\end{figure}$	Figure 1: Spectral energy distributions for 45 M 31 GCs and GC candidates.
Open with DEXTER

$\begin{figure} \par {\includegraphics[angle=-90,width=8.3cm,clip]{4157fig2.eps} } \end{figure}$	Figure 2: Graphs of the best-fit integrated colors of SSP models plotted on top of the intrinsic integrated colors for 14 GCs. Open circles with error bars represent the intrinsic integrated color of a GC, the thick line represents the best fit of the integrated color of a SSP model. The Y-axis is the ratio of the flux in each filter to the flux in filter BATC08.
Open with DEXTER

$\begin{figure} \par {\includegraphics[angle=-90,width=8.3cm,clip]{4157fig3.eps} } \par\end{figure}$	Figure 3: Contours of $\Delta \chi 2=2.30$ for a few M 31 globular clusters.
Open with DEXTER

$\begin{figure} \par {\includegraphics[angle=-90,width=8.3cm,clip]{4157fig4.eps} } \end{figure}$	Figure 4: Graphs of the best-fit integrated colors of SSP models plotted on top of the intrinsic integrated colors for 19 confirmed GCs. Open circles with error bars represent the intrinsic integrated color of an object, the thick line represents the best fit of the integrated color of a SSP model. The Y-axis is the ratio of the flux in each filter to the flux in filter BATC08.
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$\begin{figure} \par {\includegraphics[width=8.6cm,clip]{4157fig5.eps} } \end{figure}$	Figure 5: The location of the clusters ontop of M 31 image.
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$\begin{figure} \par {\includegraphics[angle=-90,width=8.8cm,clip]{4157fig6.eps} } \end{figure}$	Figure 6: Metallicity as a function of age for globular clusters of M 31.
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