A search and classification of multiple systems in the general field

Details A search and classification of multiple systems in the general field A search and classification of multiple systems in the general field

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142..103a&link_type=abstract

(IAU, Colloquium on Wide Components in Double and Multiple Stars, 97th, Brussels, Belgium, June 8-13, 1987) Astrophysics and Spa

Astronomy and Astrophysics

Astrophysics

4

Galactic Clusters, Stellar Evolution, Stellar Motions, Stellar Systems, Triple Stars, Classifications, Star Formation, Statistical Analysis

Scientific paper

Problems in the study of multiple systems of objects are reviewed, and a classification scheme for multiple star and galaxy systems is proposed. A statistical test method is used to account for uncertainties in observational data in order to determine the dynamical state of a star or galaxy system (stable or unstable). The method of simultaneously varying all the parameters observed within the limits of their errors is applied to obtain the dynamical states of eight triple stars.

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