$\begin{figure} \par\includegraphics[bb=50 50 578 578,width=12cm,clip]{0072fig1} % \end{figure}$ Figure 1: Digital Sky Survey image with all 46 stars listed in Table 2. Stars are numbered according to Siegel et al. (2001). Member stars are enclosed by boxes and other program stars indicated with crosshairs. The entire FLAMES field (diameter 26 $^\prime$ ) is shown. See Fig. 2 for a zoom into the cluster center.
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In the text

$\begin{figure} \par\includegraphics[width=15cm]{0072fig2.eps} % \end{figure}$ Figure 2: Detailed finding chart of the central field: V-band image of Palomar 13 taken with the Low-Resolution Imaging Spectrometer on the Keck II telescope from Côté et al. (2002). Member stars are enclosed by boxes and other program stars indicated with crosses.
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In the text

$\begin{figure} \par\includegraphics[bb=50 50 578 578,width=12cm,clip]{0072fig1} % \end{figure}$	Figure 1: Digital Sky Survey image with all 46 stars listed in Table 2. Stars are numbered according to Siegel et al. (2001). Member stars are enclosed by boxes and other program stars indicated with crosshairs. The entire FLAMES field (diameter 26 $^\prime$ ) is shown. See Fig. 2 for a zoom into the cluster center.
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$\begin{figure} \par\includegraphics[width=15cm]{0072fig2.eps} % \end{figure}$	Figure 2: Detailed finding chart of the central field: V-band image of Palomar 13 taken with the Low-Resolution Imaging Spectrometer on the Keck II telescope from Côté et al. (2002). Member stars are enclosed by boxes and other program stars indicated with crosses.
Open with DEXTER