Trapezium-type multiple systems

Details Trapezium-type multiple systems Trapezium-type multiple systems

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..153m&link_type=abstract

(Deutsche Forschungsgemeinschaft, Universitaet Bamberg, Universitaet Erlangen-Nuernberg, and Victoria University of Manchester,

Astronomy and Astrophysics

Astrophysics

1

Celestial Mechanics, Motion Stability, Star Clusters, Stellar Evolution, Stellar Motions, Astrometry, Orbit Decay, Star Distribution

Scientific paper

The non-stable nature of stellar motions in Trapezium-type multiple systems is discussed. The disintegration time of such systems is several orders of magnitude less than the life-time of their components, and considerably less than the disintegration time of stellar associations. The importance of ground-based and orbital observations of Trapezium-type systems is stressed.

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