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Trapezium Type Multiple Systems and Formation of Stars

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Binary and Multiple Stars as Tracers of Stellar Evolution

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 98))

Abstract

By a comparison of Trapezium-type multiple star systems in the Abastumani Catalogue and the famous Catalogue of Stellar Associations and Clusters, it is confirmed that the great number of Trapezium-type multiple stars, which belong mostly to spectral classes O-B2, are found in associations and clusters.

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References

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Author information

Authors and Affiliations

  1. Abastumani Astrophysical Observatory, USSR

    G. N. Salukvadze

Authors
  1. G. N. Salukvadze
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Editor information

Editors and Affiliations

  1. Department of Astronomy, The University, Manchester, UK

    Zdenék Kopal

  2. Dr.-Remeis-Sternwarte Bamberg, Astronomisches Institut der Universität Erlangen-Nürnberg, Germany

    Jürgen Rahe

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© 1982 D. Reidel Publishing Company

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Salukvadze, G.N. (1982). Trapezium Type Multiple Systems and Formation of Stars. In: Kopal, Z., Rahe, J. (eds) Binary and Multiple Stars as Tracers of Stellar Evolution. Astrophysics and Space Science Library, vol 98. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7861-4_13

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  • DOI: https://doi.org/10.1007/978-94-009-7861-4_13

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7863-8

  • Online ISBN: 978-94-009-7861-4

  • eBook Packages: Springer Book Archive

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