All Figures

$\begin{figure} \par\includegraphics[width=4.3cm,clip]{8845f1a}\includegraphics[w... ...idth=4.3cm,clip]{8845f1k}\includegraphics[width=4.3cm,clip]{8845f1l}\end{figure}$ Figure 1: Images of the central regions of the three galaxies of our study (NGC 2985, left; NGC 4579, centre; and NGC 4800, right). Images in the top row are in the UV (filters F218W, F250W and F300W, from left to right), the central-top row is H $\alpha$ , the central-bottom row shows the structure maps and the bottom row shows colour index images (F606W-F814W, F547M-F791W and F606W-F791W, from left to right). All images span 1 kpc on the side and the scales are such that this corresponds to 9 arcsec for NGC 2985, 12 arcsec for NGC 4579, and 13.5 arcsec for NGC 4800. The shape of the UCNR in NGC 4579, as derived from the UV image, is outlined with an ellipse. North is up and East to the left.
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In the text

$\begin{figure} \par\includegraphics[width=4.3cm,clip]{8845f2a}\includegraphics[width=4.3cm,clip]{8845f2b}\includegraphics[width=4.3cm,clip]{8845f2c}\end{figure}$ Figure 2: Close-up of the images of NGC 4800 (Fig. 1). From left to right UV, H $\alpha$ , and the structure map. The colour index image has much poorer spatial resolution and is thus not included here. All images span 0.5 kpc on the side, which corresponds to 6.7 arcsec. North is up and East to the left.
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In the text

$\begin{figure} \par\includegraphics[width=4.3cm,clip]{8845f2a}\includegraphics[width=4.3cm,clip]{8845f2b}\includegraphics[width=4.3cm,clip]{8845f2c}\end{figure}$	Figure 2: Close-up of the images of NGC 4800 (Fig. 1). From left to right UV, H $\alpha$ , and the structure map. The colour index image has much poorer spatial resolution and is thus not included here. All images span 0.5 kpc on the side, which corresponds to 6.7 arcsec. North is up and East to the left.
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