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Astron. Astrophys. 361, 1143-1151 (2000)
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Proper motions of pre-main sequence stars in southern star-forming regions * **
R. Teixeira 1,2,
C. Ducourant 2,1,
M.J. Sartori 1,
J.I.B. Camargo 1,
J.P. Périé 2,
J.R.D. Lépine 1 and
P. Benevides-Soares 1
1 Departamento de Astronomia, Universidade de São Paulo, Avenida Miguel Stéfano 4200, 04301-904 São Paulo, Brazil
2 Observatoire de Bordeaux, UMR 5804, CNRS/INSU, BP 89, 33270 Floirac, France
Received 30 March 2000 / Accepted 15 June 2000
Abstract
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
to .
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 Thé 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 213 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.
Key words: astrometry
stars:
kinematics
stars: pre-main
sequence
Galaxy: open clusters and associations: general
* Based on observations made at Valinhos CCD Meridian Circle. Based on measurements made with mama automatic measuring machine
** Table 4 is only available in electronic form at the CDS via anonymous ftp to ftp://cdsarc.u-strasbg.fr/pub/cats/J/A+A/361/1143 (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/361/1143
Send offprint requests to: teixeira@orion.iagusp.usp.br
© European Southern Observatory (ESO) 2000
Online publication: October 10, 2000
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