All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gi222_f1.ps}\end{figure}$ Figure 1: The ISGRI 25-40 keV broad view of the $\gamma$ -Cygregion (linearly scaled S/N map of the sources above 2 $\sigma$ ). The solid circle is the same as in Fig. 2.
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In the text

$\begin{figure} \par\includegraphics[width=16cm,clip]{Gi222_f2.ps} \par\end{figure}$ Figure 2: Left: ASCA GIS 6-10 keV grayscale map with an INTEGRAL ISGRI 25-40 keV 4.2 $\sigma$ contour in the NW area. Centre: ROSAT PSPC-B 0.4-2.0 keV grayscale map with the same INTEGRAL ISGRI 25-40 keV 4.2 $\sigma$ contour. Right: INTEGRAL ISGRI 25-40 keV significance map (linear scale) with H $_{\alpha }$ +[NII] 6560 Å $3\times 10^{-15}$ erg cm^-2 s^-1 arcsec^-1 contours (dotted line) and [OIII] 5010 Å $3\times 10^{-16}$ erg cm^-2 s^-1 arcsec^-1 contours (solid line) (optical data are from Mavromatakis 2003). The hard emission regions NW, NE, and SE are marked in the first two panels. The NE clump is seen with ISGRI only in the 40-80 keV band. The RXTE PCA field of view is indicated by the large solid circle. The black cross on the ROSAT map marks the position of the O9V star HD 193322 (20:18:07, +40:43:55). All maps are made for J2000.
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In the text

$\begin{figure} \includegraphics[width=0.5\textwidth,height=6.5cm,bb= 26 77 565 493,clip]{Gi222_f3.eps}\end{figure}$ Figure 3: The spectral energy distribution of the hard emission from $\gamma$ -Cyg. The ISGRI datapoints correspond to the NW clump only.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Gi222_f1.ps}\end{figure}$	Figure 1: The ISGRI 25-40 keV broad view of the $\gamma$ -Cygregion (linearly scaled S/N map of the sources above 2 $\sigma$ ). The solid circle is the same as in Fig. 2.
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$\begin{figure} \includegraphics[width=0.5\textwidth,height=6.5cm,bb= 26 77 565 493,clip]{Gi222_f3.eps}\end{figure}$	Figure 3: The spectral energy distribution of the hard emission from $\gamma$ -Cyg. The ISGRI datapoints correspond to the NW clump only.
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