All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f1.eps}\end{figure}$ Figure 1: The observed CCD field (29 $^\prime \times 18^\prime$ ) of the open cluster NGC 2126. The new variable stars are shown with open circles. Symbol sizes are proportional to the stellar brightnesses. The largest concentration of stars is about $8^\prime$ in diameter, centred at (750, 550). North is up, east is to the left.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f2.eps}\end{figure}$ Figure 2: The colour-magnitude diagrams of NGC 2126. Top row: full field of view; bottom row: the central field of 8 $^\prime$ diameter. The solid lines show the $\log t=9.1$ isochrone.
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In the text

$\begin{figure} \par\includegraphics[width=16.8cm,clip]{h4426f3.eps}\end{figure}$ Figure 3: Individual light curves of the six new variable stars. The solid lines denote Fourier fits for V3 and V5.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f4.eps}\end{figure}$ Figure 4: Phase diagrams for V1 with two equally possible periods.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f5.eps}\end{figure}$ Figure 5: The 2002 February data for V4.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{h4426f6.eps}\end{figure}$ Figure 6: Fourier analysis of V3 and V5.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f7.eps}\end{figure}$ Figure 7: Phase diagram for V6.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f8.eps}\end{figure}$ Figure 8: Outside-eclipse data folded with $P_{\rm pul}=0.12936$ d. The zero phase corresponds to a primary eclipse.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{h4426f9.eps}\end{figure}$ Figure 9: A low-resolution spectrum obtained on April 10, 2003.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{h4426f10.eps}\end{figure}$ Figure 10: Variable stars on the colour-magnitude diagram excluding foreground stars (except V6).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f1.eps}\end{figure}$	Figure 1: The observed CCD field (29 $^\prime \times 18^\prime$ ) of the open cluster NGC 2126. The new variable stars are shown with open circles. Symbol sizes are proportional to the stellar brightnesses. The largest concentration of stars is about $8^\prime$ in diameter, centred at (750, 550). North is up, east is to the left.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f2.eps}\end{figure}$	Figure 2: The colour-magnitude diagrams of NGC 2126. Top row: full field of view; bottom row: the central field of 8 $^\prime$ diameter. The solid lines show the $\log t=9.1$ isochrone.
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$\begin{figure} \par\includegraphics[width=16.8cm,clip]{h4426f3.eps}\end{figure}$	Figure 3: Individual light curves of the six new variable stars. The solid lines denote Fourier fits for V3 and V5.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f4.eps}\end{figure}$	Figure 4: Phase diagrams for V1 with two equally possible periods.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f5.eps}\end{figure}$	Figure 5: The 2002 February data for V4.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{h4426f6.eps}\end{figure}$	Figure 6: Fourier analysis of V3 and V5.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f7.eps}\end{figure}$	Figure 7: Phase diagram for V6.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{h4426f8.eps}\end{figure}$	Figure 8: Outside-eclipse data folded with $P_{\rm pul}=0.12936$ d. The zero phase corresponds to a primary eclipse.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{h4426f9.eps}\end{figure}$	Figure 9: A low-resolution spectrum obtained on April 10, 2003.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{h4426f10.eps}\end{figure}$	Figure 10: Variable stars on the colour-magnitude diagram excluding foreground stars (except V6).
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