All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig1.eps}\end{figure}$ Figure 1: APT measurements for WZ Cas. Top panel: V light change. Large symbols are APT data, small dots indicate AAVSO data (see text). Visual and photometric data typically show an offset in magnitude (see the discussion in e.g. Lebzelter & Kiss 2001). For an easier comparison the AAVSO data were scaled to the right-hand axis which is shifted slightly relatively to the left-hand axis (APT data). The shift is estimated from typical values (Lebzelter & Kiss 2001) to give an approximate fit to the APT data and should not be taken as an accurate value. Bottom panel: variation in V-I.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig2.eps} \end{figure}$ Figure 2: Comparison of light-curve data from AAVSO (open symbols) and AFOEV (filled symbols). Both datasets were subjected to an averaging procedure as described in the text.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=15cm,clip]{3076fig3.eps} \end{figure}$ Figure 3: The whole available light-curve of WZ Cas. Small dots show the measurements from the AAVSO database (see text), large dots indicate data obtained by RFG.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig4.eps} \end{figure}$ Figure 4: Variability of the most probable period of WZ Cas with time from wavelet analysis. The values for the shorter period were derived from a separate analysis with a lower maximum period limit.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig5.eps} \end{figure}$ Figure 5: First part of the velocity variations of WZ Cas on top of the AAVSO light change (small dots). Open boxes denote near-infrared measurements, filled boxes results from Coravel.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig6.eps} \end{figure}$ Figure 6: Recent velocity variations of WZ Cas ( bottom panel) compared with light variations.
Open with DEXTER

In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics*[angle=270]{3076fi7a.eps}\hspace*{2mm}\includegraphics*[angle=270]{3076fi7b.eps}} \end{figure}$ Figure 7: Two examples illustrating the change of the correlation dip. Left panel: 1999 Dec. 28 (JD 2 451 540). Right panel: 2003 May 24 (JD 2 452 783).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig8.eps} \end{figure}$ Figure 8: Variations of the shape of the correlation dip with time. Middle panel: equivalent width. Bottom panel: apparent $v\sin~i$ . Top panel: velocity variations for comparison. See text for details.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig2.eps} \end{figure}$	Figure 2: Comparison of light-curve data from AAVSO (open symbols) and AFOEV (filled symbols). Both datasets were subjected to an averaging procedure as described in the text.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15cm,clip]{3076fig3.eps} \end{figure}$	Figure 3: The whole available light-curve of WZ Cas. Small dots show the measurements from the AAVSO database (see text), large dots indicate data obtained by RFG.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig4.eps} \end{figure}$	Figure 4: Variability of the most probable period of WZ Cas with time from wavelet analysis. The values for the shorter period were derived from a separate analysis with a lower maximum period limit.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig5.eps} \end{figure}$	Figure 5: First part of the velocity variations of WZ Cas on top of the AAVSO light change (small dots). Open boxes denote near-infrared measurements, filled boxes results from Coravel.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig6.eps} \end{figure}$	Figure 6: Recent velocity variations of WZ Cas ( bottom panel) compared with light variations.
Open with DEXTER

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics[angle=270]{3076fi7a.eps}\hspace{2mm}\includegraphics*[angle=270]{3076fi7b.eps}} \end{figure}$	Figure 7: Two examples illustrating the change of the correlation dip. Left panel: 1999 Dec. 28 (JD 2 451 540). Right panel: 2003 May 24 (JD 2 452 783).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3076fig8.eps} \end{figure}$	Figure 8: Variations of the shape of the correlation dip with time. Middle panel: equivalent width. Bottom panel: apparent $v\sin~i$ . Top panel: velocity variations for comparison. See text for details.
Open with DEXTER