Astrometric study of the stellar and substellar populations of the Orion star forming region

Details Astrometric study of the stellar and substellar populations of the Orion star forming region Astrometric study of the stellar and substellar populations of the Orion star forming region

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..34...60d&link_type=abstract

IV Reunión sobre Astronomía Dinámica en Latino América (Eds. C. Allen, A. Ruelas, & R. Teixeira) Revista Mexicana de Astronomía

Astronomy and Astrophysics

Astronomy

Stars: Formation, Stars: Kinematics, Stars: Low Mass, Brown Dwarfs

Scientific paper

We present the general guidelines and first results of an astrometric project for the characterization, in terms of proper motions, of the low-mass star and substellar populations in 180 square degrees of the Orion star forming region. The first results of the astrometric reductions show coordinate uncertainties of ~ 0.004'' which, with the 10 year span of our observations, will allow for the detection of proper motions down to ~ 0.001''/year.

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