$\begin{figure} \par\includegraphics[width=8cm,clip]{aa6554f1.eps} \end{figure}$ Figure 1: (u,v) coverage of the $\eta$ Car observations. Large spots represent the UT observations and small spots the siderostat observations (North is up and East is to the right).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{aa6554f2.eps}\end{figure}$ Figure 2: Squared visibilities obtained on $\eta$ Car with VINCI, compared to the model fitting result of Weigelt et al. (2007), represented as a solid curve. The UT data points are represented with open squares.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{aa6554f1.eps} \end{figure}$	Figure 1: (u,v) coverage of the $\eta$ Car observations. Large spots represent the UT observations and small spots the siderostat observations (North is up and East is to the right).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{aa6554f2.eps}\end{figure}$	Figure 2: Squared visibilities obtained on $\eta$ Car with VINCI, compared to the model fitting result of Weigelt et al. (2007), represented as a solid curve. The UT data points are represented with open squares.
Open with DEXTER