  In this publication we present a study of the general physical, chemical
properties and radial velocity monitoring of young active stars. We derive
temperatures, log g, [Fe/H], v sin i, and R_{spec} values for eight stars. The
detailed analysis reveals that the stars are not as homogeneous in their
premier physical parameters as well as in the age distribution. In 4/5 we found
a periodic radial velocity signal which origins in surface features the fifth
is surprisingly inactive and shows little variation.
