I will present the results of planet searches around nearby young stars with the radial 
velocity technique by using FEROS at 2.2 m MPG/ESO telescope.
During our observations from 2003 until 2006 we found evidence for planetary companions 
around young (30 - 300 Myrs) stars. The radial velocity variation of the planet host stars 
have periodicities of several hundred of days which are significantly longer than the 
stellar rotational periods. The positive detections have been confirmed by the lack of 
correlation between the bisector velocity spans and radial velocities.