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.
@article{arxiv.astro-ph/0207078,
title = {SACY - Present Status},
author = {C. A. O. Torres and G. R. Quast and R. de la Reza and L. da Silva and C. H. F. Melo},
journal= {arXiv preprint arXiv:astro-ph/0207078},
year = {2016}
}