$\begin{figure} \par\includegraphics[width=8.6cm,clip]{8737fig1.ps} \includegraphics[width=8.4cm,clip]{8737fig2.ps}\end{figure}$ Figure 1: Radial-velocity measurements as a function of Julian Date obtained with CORALIE for HD 4113, superimposed on the best Keplerian planetary solution (top figure). The residuals are displayed at the bottom of the top figure, and the phase folded radial-velocity measurements are displayed on the bottom diagram.
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In the text

$\begin{figure} \par\includegraphics[width=6.6cm,clip]{8737fig5.ps} \end{figure}$ Figure 3: e vs. $\log{P}$ for the known extra-solar giant planets orbiting dwarf primaries. Filled dots are for planets orbiting single stars and open squares for planets orbiting a component of a multiple stellar system. Green stars correspond to stars hosting Netpune-like planets. HD 4113 b and HD 156846 b are located by filled red squares.
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In the text

$\begin{figure} \par\includegraphics[width=8.6cm,clip]{8737fig1.ps} \includegraphics[width=8.4cm,clip]{8737fig2.ps}\end{figure}$	Figure 1: Radial-velocity measurements as a function of Julian Date obtained with CORALIE for HD 4113, superimposed on the best Keplerian planetary solution (top figure). The residuals are displayed at the bottom of the top figure, and the phase folded radial-velocity measurements are displayed on the bottom diagram.
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$\begin{figure} \par\includegraphics[width=8.5cm,clip]{8737fig3.ps} \includegraphics[width=8.4cm,clip]{8737fig4.ps} \end{figure}$	Figure 2: Same as Fig. 1 for HD 156846.
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$\begin{figure} \par\includegraphics[width=6.6cm,clip]{8737fig5.ps} \end{figure}$	Figure 3: e vs. $\log{P}$ for the known extra-solar giant planets orbiting dwarf primaries. Filled dots are for planets orbiting single stars and open squares for planets orbiting a component of a multiple stellar system. Green stars correspond to stars hosting Netpune-like planets. HD 4113 b and HD 156846 b are located by filled red squares.
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