All Figures

$\begin{figure} \par\includegraphics[width=15cm,clip]{9732fig1.eps}\end{figure}$ Figure 1: The central $18''\times 18''$ region of NGC 1808 (1''=53 pc). The axis units are arcsec. The nucleus (source M 1) is positioned at coordinates (0''; 0''). North is up and East is to the left. The MIR sources are labelled as in Galliano et al. (2005) on the TIMMI2 map. Zooms towards the two regions delimited by the squares (Regions A and B) are displayed in Fig. 2. The long rectangles feature the spectroscopic slits: small ticks are spaced by 1'', while long thick ticks highlight the positions at which line emission has been recorded.
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In the text

$\begin{figure} \par\includegraphics[width=18cm,clip]{9732fig2.eps}\end{figure}$ Figure 2: Zooms towards regions A and B of the NGC 1808 central starburst. These regions are defined in Fig. 1. The axis units are arcsec, North is up and East is to the left. Regarding the slit drawings, see the caption of Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[width=14cm,clip]{9732fig3.eps}\end{figure}$ Figure 3: ISAAC spectra of the MIR/radio sources M 1, M 3, M 6 and M 8 in the central region of NGC 1808. The slit positions, as well as the source positions along the slits are shown in Figs. 1 and 2.
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{9732fig4.eps}\end{figure}$ Figure 4: Position-velocity diagram for Br ${\gamma }$ along the slit which contains the two embedded clusters M 6 and M 8. The X-axis shows the wavelength expressed in relative radial velocity in $\rm ~km~s^{-1}$ and the Y-axis gives the relative angular position in arcsec.
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In the text

$\begin{figure} \par\includegraphics[width=18cm,clip]{9732fig2.eps}\end{figure}$	Figure 2: Zooms towards regions A and B of the NGC 1808 central starburst. These regions are defined in Fig. 1. The axis units are arcsec, North is up and East is to the left. Regarding the slit drawings, see the caption of Fig. 1.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{9732fig3.eps}\end{figure}$	Figure 3: ISAAC spectra of the MIR/radio sources M 1, M 3, M 6 and M 8 in the central region of NGC 1808. The slit positions, as well as the source positions along the slits are shown in Figs. 1 and 2.
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$\begin{figure} \par\includegraphics[width=6cm,clip]{9732fig4.eps}\end{figure}$	Figure 4: Position-velocity diagram for Br ${\gamma }$ along the slit which contains the two embedded clusters M 6 and M 8. The X-axis shows the wavelength expressed in relative radial velocity in $\rm ~km~s^{-1}$ and the Y-axis gives the relative angular position in arcsec.
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