  The purpose of this study is the identification of young ($1< age < 100$
Myr), nearby ($d \leqslant100$ pc) moving groups (YNMGs) through their
kinematic signature. YNMGs could be the result of the recent dispersal of young
embedded clusters, such that they still represent kinematically cold groups,
carrying the residual motion of their parental cloud. Using the fact that a
large number ($\sim$ 14000) of the RAVE sources with evidence of chromospheric
activity, also present signatures of stellar youth, we selected a sample of
solar type sources with the highest probability of chromospheric activity to
look for common kinematics. We made use of radial velocity information from
RAVE and astrometric parameters from GAIA DR2 to construct a 6-dimension
position-velocity vector catalog for our full sample. We developed a method
based on the grouping of stars with similar orientation of their velocity
vectors, which we call the Cone Method Sampling. Using this method, we detected
646 sources with high significance in the velocity space, with respect to the
average orientation of artificial distributions made from a purely Gaussian
velocity ellipsoid with null vertex deviation. We compared this sample of
highly significant sources with a catalog of YNMGs reported in previous
studies, which yield 75 confirmed members. From the remaining sample, about 50%
of the sources have ages younger than 100 Myr, which indicate they are highly
probable candidates to be new members of identified or even other YNMGs in the
solar neighborhood.
