Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8cm,clip]{2003_0303_f1.eps}\end{figure}$ Figure 1: Power density spectrum of M 33 X-8 build from all the XMM-Newton observations, except for ObsID 0102640101, which showed instrumental noise.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2003_0303_f2.eps}\end{figure}$ Figure 2: Global light curve of M 33 X-8 (all the observations) folded with a period of 5000 s. Error bars are at $1\sigma$ .
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.2cm,clip]{2003_0303_f3.eps}\\ \includegraphics[angle=270,width=8.3cm,clip]{2003_0303_f4.eps}\end{figure}$ Figure 3: (top) Best-fit spectrum of M 33-X8 with EPIC MOS1, MOS2, and PN data. The model used is the multicolour disc plus a power law. See Table 2 and the text for details. The ratio data/model is shown in the bottom panel. (bottom)Corresponding unfolded spectrum.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.15cm,clip]{2003_0303_f5.eps}\end{figure}$ Figure 4: 2-dimensional fit-statistic contour plot of $\Gamma$ versus $N_{\rm H}$ . The contours are with $\Delta \chi ^2=2.3, 4.61, 9.21$ , corresponding to the confidence levels of 68%, 90%, and 99%.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2003_0303_f1.eps}\end{figure}$	Figure 1: Power density spectrum of M 33 X-8 build from all the XMM-Newton observations, except for ObsID 0102640101, which showed instrumental noise.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{2003_0303_f2.eps}\end{figure}$	Figure 2: Global light curve of M 33 X-8 (all the observations) folded with a period of 5000 s. Error bars are at $1\sigma$ .
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=270,width=8.2cm,clip]{2003_0303_f3.eps}\\ \includegraphics[angle=270,width=8.3cm,clip]{2003_0303_f4.eps}\end{figure}$	Figure 3: (top) Best-fit spectrum of M 33-X8 with EPIC MOS1, MOS2, and PN data. The model used is the multicolour disc plus a power law. See Table 2 and the text for details. The ratio data/model is shown in the bottom panel. (bottom)Corresponding unfolded spectrum.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=270,width=8.15cm,clip]{2003_0303_f5.eps}\end{figure}$	Figure 4: 2-dimensional fit-statistic contour plot of $\Gamma$ versus $N_{\rm H}$ . The contours are with $\Delta \chi ^2=2.3, 4.61, 9.21$ , corresponding to the confidence levels of 68%, 90%, and 99%.
Open with DEXTER