All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{6110fig1.ps} \end{figure}$ Figure 1: The flux-calibrated spectrum of TV Ret taken in September 2003. The upper plot shows the full intensity range; in the lower plot the intensity range has been decreased to better display the weak emission lines and the slope of the continuum.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{6110fig2.ps} \end{figure}$ Figure 2: The spectrum of TV Ret taken in November 2004 with the continuum normalised to unity. The upper plot shows the full intensity range; in the lower plot the intensity range has been decreased to better display the weak emission lines.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6110fig3.ps} \end{figure}$ Figure 3: The R-band acquisition image shows the $3 \times 3$ arcmin surroundings of TV Ret ( in the centre) and a zoom on the object; north is up, east is left. With the good seeing of 0.6'' the object appears clearly extended. On the right side, the contours of TV Ret ( upper plot) and a star for comparison are plotted.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{6110fig4.ps} \end{figure}$ Figure 4: The B-magnitude of TV Ret plotted against the heliocentric Julian Date. The data are taken from Table 5 of Kinman et al. (1991). The smaller plot is a zoom on the last 40 days, when the outburst happened.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{6110fig1.ps} \end{figure}$	Figure 1: The flux-calibrated spectrum of TV Ret taken in September 2003. The upper plot shows the full intensity range; in the lower plot the intensity range has been decreased to better display the weak emission lines and the slope of the continuum.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{6110fig2.ps} \end{figure}$	Figure 2: The spectrum of TV Ret taken in November 2004 with the continuum normalised to unity. The upper plot shows the full intensity range; in the lower plot the intensity range has been decreased to better display the weak emission lines.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{6110fig3.ps} \end{figure}$	Figure 3: The R-band acquisition image shows the $3 \times 3$ arcmin surroundings of TV Ret ( in the centre) and a zoom on the object; north is up, east is left. With the good seeing of 0.6'' the object appears clearly extended. On the right side, the contours of TV Ret ( upper plot) and a star for comparison are plotted.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{6110fig4.ps} \end{figure}$	Figure 4: The B-magnitude of TV Ret plotted against the heliocentric Julian Date. The data are taken from Table 5 of Kinman et al. (1991). The smaller plot is a zoom on the last 40 days, when the outburst happened.
Open with DEXTER