Fig. 4

Radial velocity observations and orbital solution of HD 196885 AB based on the CORAVEL, ELODIE, CORALIE and Lick surveys. Top Left: radial velocity variation as a function of time with the best orbital solution overplotted presenting the complete set of RV observations. Top Right: zoom-in on the RV variation due to the giant planet HD 196885 Aa superimposed to the RV drift due to the companion HD 196885 B. Bottom Left: radial velocity variation of HD 196885 A due to the B component only as a function of the orbital phase. Bottom Right: radial velocity variation of HD 196885 A due to the Ab planet only as a function of the orbital phase.
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