  We review topics related to the dispersal of young stars from their
birth-sites, and focus in particular on the entourage of young stars related to
the ongoing star-formation event in the Sco-Cen OB association. We conduct a
follow-up kinematic study to that presented in Mamajek, Lawson, & Feigelson
(2000; ApJ 544, 356) amongst nearby, isolated, young stars. In addition to the
eta Cha and TW Hya groups, we find several more intriguing Sco-Cen outlier
candidates: most notably beta Pic, PZ Tel, HD 199143, and HD 100546. We discuss
the connection between Sco-Cen and the southern ``150 pc Conspiracy'' molecular
clouds, and in particular, Corona Australis. The kinematic evidence suggests
that many of the nearby, isolated ~10 Myr-old stars were born near Sco-Cen
during the UCL and LCC starbursts 10-15 Myr ago. We hypothesize that these
stars inherited 5-10 km/s velocities moving away from Sco-Cen, either through
molecular cloud turbulence, or through formation in molecular clouds associated
with the expanding Sco-Cen superbubbles (e.g. Loop I).
