  The scientific goal of the SACY (Search for Associations Containing
Young-stars) project is to identify eventual associations of stars younger than
the Local Association, spread among the optical counterparts of the ROSAT X-ray
bright sources. High-resolution spectra for possible optical counterpart later
than G0 belonging to HIPPARCOS and/or TYCHO-2 catalogues were obtained in order
to assess both the youth and the spatial motion of each target. The newly
identified young stars present a patchy distribution in UVW space and in the
sky as well revealing the existence of huge nearby young associations. Here we
present the associations identified in the present sample.
