  We present proper motion measurements of pre-main sequence (PMS) stars
associated with major star-forming regions of the southern hemisphere
(Chamaeleon, Lupus, Upper Scorpius - Ophiuchus, Corona Australis), situated in
the galactic longitude range l = 290\degr to l = 360\degr. A list of PMS stars
as complete as possible was established based on the Herbig and Bell catalogue
and many new catalogues like the PDS survey, the catalogue of Herbig Ae/Be
stars by Th\'e et al. (1994), X-rays surveys, etc. The measurements made use of
public material (mainly AC2000 and USNO--A2.0 catalogues) as well as scans of
SERC-J Schmidt plates with the MAMA measuring machine (Paris) and Valinhos CCD
meridian circle observations (Brazil). We derived proper motions for 214 stars,
with an accuracy of 5 to 10 mas/yr depending mainly on the difference of epochs
between the position sources. The main characteristics of the sample are
discussed. We show that systematic motions of groups of stars exist, which are
not explained by the reflex solar motion.
