Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-23T02:56:08.846Z Has data issue: false hasContentIssue false
  • English
  • Français

Eclipsing Binaries in Multiple Star Systems

Published online by Cambridge University Press:  07 August 2017

C. R. Chambliss
C. R. Chambliss*
Affiliation:
Kutztown University, Kutztown, Pennsylvania, USA 19530

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Although the majority of the known eclipsing binaries are in systems which consist of only the two eclipsing components, a significant number of them do occur as components of triple star systems or higher order multiple star systems. In this context this term is restricted to those systems whose components are in closed orbits. A recent survey of visual binaries with variable components is that by Proust et al. (1981), which details about 300 systems. Walker (1979) has also prepared a list of variables as components of double star systems, and this includes numerous systems not included in other lists.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 315 - 318
Copyright
Copyright © Kluwer 1992 

References

Fekel, F. C. (1981), Astrophys. J. 246, 879.CrossRefGoogle Scholar
Proust, D. Ochsenbein, F., and Pettersen, B. R. (1981), Astron. Astrophys. Suppl. Ser. 44, 179.Google Scholar
Walker, R. L. (1979), A Catalog of Visual Binaries with One or More Variable Components, unpublished.Google Scholar