All Figures

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4960fig1.eps} \end{figure}$ Figure 1: Finding chart of the WFPC2 fields considered for this work. The region is $20'\times 20'$ wide and is centered on the center of NGC 6397. The fields measured in this work are labeled "B'',"C'', and "D''. For completeness we also show field "A'', which we did not use here (see text) but will use in forthcoming papers. Fields A, B, C, D are centered 5', 4 $.\mkern -4mu^\prime$ 5, 8', and 8' from the cluster center, respectively.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4960fig2.eps} \end{figure}$ Figure 2: Vector-point diagram of the proper motions in equatorial coordinates, combining all the fields. Open circles with error bars represent the selected reference galaxies. Dots represent the stars; a circle at 3 mas/yr separates cluster members from field objects. The arrow is the adopted absolute proper motion of NGC 6397.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4960fig3.eps} \end{figure}$ Figure 3: Spatial distribution of stars with radial velocity measurement. The circles indicate the radial distances of 5 and 10 arc min from the center of the cluster.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4960fig4.eps} \end{figure}$ Figure 4: Radial velocities of the observed sample of stars as a function of magnitude.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4960fig5.eps}\protect\end{figure}$ Figure 5: Calculated orbits for assumed distances 1.8, 2.0, 2.2, and 2.4 kpc.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4960fig2.eps} \end{figure}$	Figure 2: Vector-point diagram of the proper motions in equatorial coordinates, combining all the fields. Open circles with error bars represent the selected reference galaxies. Dots represent the stars; a circle at 3 mas/yr separates cluster members from field objects. The arrow is the adopted absolute proper motion of NGC 6397.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4960fig3.eps} \end{figure}$	Figure 3: Spatial distribution of stars with radial velocity measurement. The circles indicate the radial distances of 5 and 10 arc min from the center of the cluster.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{4960fig4.eps} \end{figure}$	Figure 4: Radial velocities of the observed sample of stars as a function of magnitude.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{4960fig5.eps}\protect\end{figure}$	Figure 5: Calculated orbits for assumed distances 1.8, 2.0, 2.2, and 2.4 kpc.
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