All Figures

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{9843fig1.ps} \end{figure}$ Figure 1: Average spectrum of NSV 13983. The large artifact at $\sim$ 5016 $\AA$ could not be corrected due to its proximity to a He I line.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{9843fig2.ps} \end{figure}$ Figure 2: Scargle periodgram for H $\alpha$ . The peak corresponds to P = 2.76 h.
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{9843fig3.ps} \end{figure}$ Figure 3: Radial velocities of H $\alpha$ ( top) and H $\beta$ (bottom) versus orbital phase. The data are represented in the order of their observation, i.e. phase 0 is set to be the first observed data point, and the last observation corresponds to phase 1.11. The solid curve represents the best fit with respect to P = 2.76 h.
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{9843fig4.ps} \end{figure}$ Figure 4: Close-up of the period distribution of CVs about the period gap, based on version 7.9 of the Ritter & Kolb (2003) catalogue, excluding objects of uncertain period (i.e., those marked with a colon). Two distributions are shown: all CV subtypes (light grey) and dwarf novae only (dark grey). The dashed lines mark the limits of the period gap defined by Knigge (2006). The bin size is 0.02 units. The arrow marks the position of NSV 13983, which is not included in the histograms.
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{9843fig1.ps} \end{figure}$	Figure 1: Average spectrum of NSV 13983. The large artifact at $\sim$ 5016 $\AA$ could not be corrected due to its proximity to a He I line.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{9843fig2.ps} \end{figure}$	Figure 2: Scargle periodgram for H $\alpha$ . The peak corresponds to P = 2.76 h.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{9843fig3.ps} \end{figure}$	Figure 3: Radial velocities of H $\alpha$ ( top) and H $\beta$ (bottom) versus orbital phase. The data are represented in the order of their observation, i.e. phase 0 is set to be the first observed data point, and the last observation corresponds to phase 1.11. The solid curve represents the best fit with respect to P = 2.76 h.
Open with DEXTER