$\begin{figure} \par\includegraphics[width=8.8cm,clip]{bedin_f4.eps} \end{figure}$ Figure 4: Example of radius determination for the first four clusters in the catalog presented in this work. For each cluster, the radius was obtained with three different methods (see the text).
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=4cm,clip]{41_CS82.eps}\hspace*{1... ...pace*{1mm}\includegraphics[width=4cm,clip]{H9_CS82.eps} } \protect \end{figure}$ Figure 5: ( Top panels) The two cluster candidates labeled in CS82 as $\char93 41$ and $\char93 42$ , were confirmed in this work to be star clusters; namely: 24, 22 according to IDs given in Table 1. ( Bottom panels) Also, the two HII regions labeled in CS82 as H $\char93$ 8 and H $\char93 9$ were confirmed in this work to be star clusters, whose IDs are 4, 25, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,angle=-90,clip]{bedin_f1.eps} \end{figure}$ Figure 1: WFC/ACS field finding chart. The field of view is $40'\times 40'$ , North on top, and East to the left.
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In the text

$\begin{figure} \par\includegraphics[width=20cm,angle=90,clip]{bedin_f2.eps} \end{figure}$ Figure 2: Cluster identification charts for WFC/ACS top chip. Squares indicate the new clusters (Table 1), circles mark background galaxies (Table 2) and cluster candidates (Table 3). Triangles indicate the presence of gas or of diffuse objects.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{bedin_f4.eps} \end{figure}$	Figure 4: Example of radius determination for the first four clusters in the catalog presented in this work. For each cluster, the radius was obtained with three different methods (see the text).
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$\begin{figure} \par\mbox{\includegraphics[width=4cm,clip]{41_CS82.eps}\hspace{1... ...pace{1mm}\includegraphics[width=4cm,clip]{H9_CS82.eps} } \protect \end{figure}$	Figure 5: ( Top panels) The two cluster candidates labeled in CS82 as $\char93 41$ and $\char93 42$ , were confirmed in this work to be star clusters; namely: 24, 22 according to IDs given in Table 1. ( Bottom panels) Also, the two HII regions labeled in CS82 as H $\char93$ 8 and H $\char93 9$ were confirmed in this work to be star clusters, whose IDs are 4, 25, respectively.
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$\begin{figure} \par\begin{tabular}{ccc} \fbox{\includegraphics[width=5cm]{bedin_... ...{\includegraphics[width=5cm]{bedin_F.eps}}\\ \end{tabular}\protect \end{figure}$	Figure 6: Example of galaxy (51), populous cluster (31), compact (9), populous (7), low density + HII(8), association (12), and HII shell structure (34).
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$\begin{figure} \par\includegraphics[width=8.8cm,angle=-90,clip]{bedin_f1.eps} \end{figure}$	Figure 1: WFC/ACS field finding chart. The field of view is $40'\times 40'$ , North on top, and East to the left.
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$\begin{figure} \par\includegraphics[width=20cm,angle=90,clip]{bedin_f2.eps} \end{figure}$	Figure 2: Cluster identification charts for WFC/ACS top chip. Squares indicate the new clusters (Table 1), circles mark background galaxies (Table 2) and cluster candidates (Table 3). Triangles indicate the presence of gas or of diffuse objects.
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$\begin{figure} \par\includegraphics[width=20cm,angle=90,clip]{bedin_f3.eps} \end{figure}$	Figure 3: Cluster identification charts for WFC/ACS bottom chip. Symbols as in Fig. 2.
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