![\begin{figure}
\par\includegraphics[width=7.8cm,clip]{09402F1.eps}\end{figure}](/articles/aa/full/2008/31/aa09402-08/img5.gif) |
Figure 1: Spectral region of HD 45652 centered at the Ca II K line (CORALIE spectrum). |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.7cm,clip]{09402F2.eps}\end{figure}](/articles/aa/full/2008/31/aa09402-08/img18.gif) |
Figure 2: Top: ELODIE (red circles), CORALIE (blue squares), and SOPHIE (magenta diamonds) radial-velocities for HD 45652 as a function of time, and the best-fit Keplerian function to the data. Bottom: residuals of the fit. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.9cm,clip]{09402F3.eps}\end{figure}](/articles/aa/full/2008/31/aa09402-08/img19.gif) |
Figure 3: Phase-folded ELODIE, CORALIE, and SOPHIE radial velocities for HD 45652 at a period of 43.6 days. Symbols are as in Fig. 2. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.1cm,clip]{09402F4.eps}\end{figure}](/articles/aa/full/2008/31/aa09402-08/img24.gif) |
Figure 4:
BIS versus radial-velocity for the CORALIE data of HD 45652. To
demonstrate the nonexistence of a correlation, the vertical and
horizontal scales were set to be identical. The best linear fit to the data
is also shown. The slope of the fit has a non significant value of
0.02  0.09. |
| Open with DEXTER | |
In the text