Dynamical 3-D evolution of nearby young moving groups

Details Dynamical 3-D evolution of nearby young moving groups Dynamical 3-D evolution of nearby young moving groups

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26...91o&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Using 3-D trajectories of probable members of previously photometrically and spectroscopically studied stellar moving groups β Pictoris, TW Hya, η Chamaeleontis, ɛ Chamaeleontis, we confirmed the star memberships and determined dynamical ages. Only stars with complete kinematical data (Hipparcos astrometry and radial velocities) were taken into consideration. The observed temporal sequence of group formation is consistent with the existence of a wave of star formation in the Scorpio-Centaurus OB association region.

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