Trapezium-type multiple systems

Details Trapezium-type multiple systems Trapezium-type multiple systems

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..321s&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

B Stars, Binary Stars, O Stars, Star Clusters, Statistical Analysis

Scientific paper

Trapezium-type multiple systems are one of the youngest systems in the galaxy. Ambartsumian (1954) regards many of the Trapezium-type multiple systems as having positive total energy. The examination of a table, compiled from the Abastumani Catalogue of Trapezia (Salukvadze, 1978; Poveda et al., 1977) and the Index Catalogue of Visual Binary Stars, shows that real trapezia are met among multiple stars with their primaries of O and B spectral types.

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