All Figures

$\begin{figure} \par\includegraphics[width=7cm,clip]{AA1121_fig1.eps} \end{figure}$ Figure 1: Distribution of stars from the USNO-B1 catalogue in a 20' $\times$ 20' field around NGC 5385. The sizes of the dots are proportional to the magnitudes of the stars.
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In the text

$\begin{figure} \par\includegraphics[height=9.65cm,width=7.85cm,clip]{AA1121_fig2.eps} \end{figure}$ Figure 2: Histogram of the surface density of the stars shown in Fig. 1, measured by counts in $0\hbox {$.\mkern -4mu^\prime $ }5$ wide annuli centered on $\alpha =13^{\rm h}52^{\rm m}19^{\rm s}$ , $\delta =+76^{\circ }10'56''$ . Dots with error bars indicate the mean surface density of stars in a nearby field centered on $\alpha =13^{\rm h}54^{\rm m}10^{\rm s}$ , $\delta =+76^{\circ }49'30''$ , and the expected 1 $\sigma$ range of statistical fluctuations around this mean for each bin.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{AA1121_fig3.eps} \end{figure}$ Figure 3: Distribution of stars from the UCAC2 catalogue in a 30' $\times$ 30' field around NGC 2664. The sizes of the dots are proportional to the magnitudes of the stars.
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In the text

$\begin{figure} \par\includegraphics[height=9.65cm,width=7.9cm,clip]{AA1121_fig4.eps} \end{figure}$ Figure 4: Histogram of the surface densities of the stars shown in Fig. 3, measured by counts in $0\hbox {$.\mkern -4mu^\prime $ }5$ wide annuli centered on $\alpha =08^{\rm h}47^{\rm m}07^{\rm s}$ , $\delta =+12^{\circ }36'30''$ . Dots with error bars indicate the mean surface density of stars in a nearby field centered on $\alpha =08^{\rm h}53^{\rm m}05^{\rm s}$ , $\delta =+12^{\circ }59'50''$ , and the expected 1 $\sigma$ range of statistical fluctuations around this mean for each bin.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{AA1121_fig5.eps} \end{figure}$ Figure 5: Distribution of stars from the UCAC2 catalogue in a 30' $\times$ 30' field around Collinder 21. The sizes of the dots are proportional to the magnitudes of the stars.
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In the text

$\begin{figure} \par\includegraphics[height=9.65cm,width=7.85cm,clip]{AA1121_fig6.eps} \end{figure}$ Figure 6: Histogram of the surface densities of the stars shown in Fig. 5, measured by counts in $0\hbox {$.\mkern -4mu^\prime $ }5$ wide annuli centered on $\alpha =01^{\rm h}50^{\rm m}11^{\rm s}$ , $\delta =+27^{\circ }04'26''$ . Dots with error bars indicate the mean surface density of stars in a nearby field centered on $\alpha =01^{\rm h}54^{\rm m}10^{\rm s}$ , $\delta =+27^{\circ }44'00''$ , and the expected 1 $\sigma$ range of statistical fluctuations around this mean for each bin.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{AA1121_fig7.eps}\end{figure}$ Figure 7: Identification map ( $8\hbox {$.\mkern -4mu^\prime $ }14$ $\times$ $8\hbox {$.\mkern -4mu^\prime $ }14$ ), taken from DSS-2) for member candidates of NGC 5385 for which there are proper motions measurements from Tycho 2. North is up, East on the left. The labels give the star numbers assigned in the Tycho-2 catalog (in the sense TYC 4558-<...>).The data for these stars are given in Tables 3 and 6.
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In the text

$\begin{figure} \par\includegraphics[width=16cm,clip]{AA1121_fig8.eps}\end{figure}$ Figure 8: Photometry and proper motions in the region of NGC 5385. a) Color-magnitude diagram. Open squares are Tycho 2 stars for which there are both proper motion and radial velocity measurements (see panel b) and Table 6), while filled triangles are stars having only proper motion measurements. b) Vector point plot of Tycho 2 proper motions and proper motion errors. Symbols are as in panel a). The identification numbers are from Tycho 2. See text for more details.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{AA1121_fig9.eps}\end{figure}$ Figure 9: Identification map ( $8\hbox {$.\mkern -4mu^\prime $ }14$ $\times$ $8\hbox {$.\mkern -4mu^\prime $ }14$ , taken from DSS-2) for member candidates of NGC 2664 for which there are proper motions measurements from Tycho 2. North is up, East on the left. The labels give the star numbers assigned in the Tycho-2 catalog (in the sense TYC 816-<...>. The data for these stars are given in Tables 4 and 7.
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In the text

$\begin{figure} \par\includegraphics[width=15.7cm,clip]{AA1121_fig10.eps}\end{figure}$ Figure 10: Photometry and proper motions in the region of NGC 2664. a) Color-magnitude diagram. Open squares are Tycho 2 stars for which there are both proper motion and radial velocity measurements (see panel b) and Table 7), while filled triangles are stars for which there are only proper motion measurements. b) Vector point plot of Tycho 2 proper motions and proper motion errors. Symbols are as in panel a).The identification numbers are from Tycho 2. See text for more details.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{AA1121_fig11.eps}\end{figure}$ Figure 11: Identification map ( $8\hbox {$.\mkern -4mu^\prime $ }14$ $\times$ $8\hbox {$.\mkern -4mu^\prime $ }14$ , taken from DSS-2) for member candidates of Collinder 21 for which there are proper motion measurements from Tycho 2. North is up, East on the left. The labels give the star numbers assigned in the Tycho-2 catalog (in the sense TYC 1759-<...>). The data for these stars are given in Tables 5 and 8.
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In the text

$\begin{figure} \par\includegraphics[width=15.6cm,clip]{AA1121_fig12.eps}\end{figure}$ Figure 12: Photometry and proper motions in the region of Collinder 21. a) Color-magnitude diagram. Open squares are Tycho 2 stars having both proper motion and radial velocity measurements (see panel b) and Table 8), while filled triangles are stars for which there are only proper motion measurements. b) Vector point plot of Tycho 2 proper motions and proper motion errors. Symbols are as in panel a). The identification numbers are from Tycho 2. See text for more details.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{AA1121_fig1.eps} \end{figure}$	Figure 1: Distribution of stars from the USNO-B1 catalogue in a 20' $\times$ 20' field around NGC 5385. The sizes of the dots are proportional to the magnitudes of the stars.
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$\begin{figure} \par\includegraphics[width=7cm,clip]{AA1121_fig3.eps} \end{figure}$	Figure 3: Distribution of stars from the UCAC2 catalogue in a 30' $\times$ 30' field around NGC 2664. The sizes of the dots are proportional to the magnitudes of the stars.
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$\begin{figure} \par\includegraphics[width=7cm,clip]{AA1121_fig5.eps} \end{figure}$	Figure 5: Distribution of stars from the UCAC2 catalogue in a 30' $\times$ 30' field around Collinder 21. The sizes of the dots are proportional to the magnitudes of the stars.
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