Adaptive Optics Survey of Young and Nearby Associations

Details Adaptive Optics Survey of Young and Nearby Associations Adaptive Optics Survey of Young and Nearby Associations

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..437c&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Physics

Optics

Scientific paper

Young and Nearby stellar associations became of particular interest over the past few years as ideal targets to search for low-mass companions and/or circumstellar disks. The detection of young sub-stellar objects and proto-planetary disks id crucial to constrain the current models of planetary formation, and improve our understanding of the physical processes involved. In such exciting context, I will present the results of the adaptive optics surveys of three Young Associations : Capricornus, MBM 12 and the Tucana-HorologiumiA.

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