On the Origin of the Very Young Groups η and epsilon Chamaeleontis

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© 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation E. Jilinski et al 2005 ApJ 619 945 DOI 10.1086/426535

0004-637X/619/2/945

Abstract

The three-dimensional orbits of the kinematical centers of the η Cha and epsilon Cha compact groups are retraced under the action of a general Galactic potential. The results show that both groups were formed in the same spatial region about 7 Myr ago. Their birthplace appears to be quite near the Lower Centaurus Crux subgroup of the Sco-Cen OB association. The epoch of minimum separation in the past between η Cha and epsilon Cha turns out to be consistent with the estimated evolutionary age.

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10.1086/426535