All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{3683f1.ps} \end{figure}$ Figure 1: Data to power law plus Galactic absorption model ratio.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{3683f2.ps} \end{figure}$ Figure 2: Confidence contours of the Fe K $\alpha$ line versus its width (sigma). The line is consistent with being narrow at 99% confidence level.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{3683f3.ps} \end{figure}$ Figure 3: Broad band (0.5-100 keV) spectrum of MKN6 fitted with model 3 of Table 1.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.1cm,clip]{3683f4.ps} \end{figure}$ Figure 4: LECS+MECS BeppoSAX data fitted with model 3 but imposing the best fit parameters obtained by ASCA for both partial covering absorbers.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.5cm,clip]{3683f5.ps} \end{figure}$ Figure 5: Comparison of the column densities found by ASCA (dashed lines) and BeppoSAX (solid lines).
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In the text