All Figures

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{7508fig1.eps} \end{figure}$ Figure 1: Lightcurves at periastron ( top) and apastron ( bottom). The average value is given as a long-dashed line. The time axis is different for each lightcurve.
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In the text

$\begin{figure} \par\includegraphics[angle=0, width=8cm]{7508fig2.eps} \end{figure}$ Figure 2: Spectral data from pn ( upper spectrum), MOS1 and MOS2 ( lower spectra) cameras, and the best fit to the three of them: an absorbed power-law, around phase 0.5 (those around phase 0.0 look very similar and are not shown here). The deviations in $\sigma$ of the model from the data are shown in the lower panel.
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In the text

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{7508fig3.eps}} \end{figure}$ Figure 3: The year averages (black circles) and the individuals points (white squares) for the H ${\alpha }$ EW. For those years with several data points, the year average points are shown and their error bars represent the dispersion of values. The data come from this and previous works (C05: 2003; MS04: 1998, 1999, 2000, 2003; R03: 1999, 2002).
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{7508fig1.eps} \end{figure}$	Figure 1: Lightcurves at periastron ( top) and apastron ( bottom). The average value is given as a long-dashed line. The time axis is different for each lightcurve.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=0, width=8cm]{7508fig2.eps} \end{figure}$	Figure 2: Spectral data from pn ( upper spectrum), MOS1 and MOS2 ( lower spectra) cameras, and the best fit to the three of them: an absorbed power-law, around phase 0.5 (those around phase 0.0 look very similar and are not shown here). The deviations in $\sigma$ of the model from the data are shown in the lower panel.
Open with DEXTER

$\begin{figure} \par\resizebox{8.8cm}{!}{\includegraphics{7508fig3.eps}} \end{figure}$	Figure 3: The year averages (black circles) and the individuals points (white squares) for the H ${\alpha }$ EW. For those years with several data points, the year average points are shown and their error bars represent the dispersion of values. The data come from this and previous works (C05: 2003; MS04: 1998, 1999, 2000, 2003; R03: 1999, 2002).
Open with DEXTER