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The Age of the Triple System HD 165590

Published online by Cambridge University Press:  12 April 2016

Gustav A. Bakos  and
Jozef Tremko
Gustav A. Bakos
Affiliation:
Department of Physics, University of Waterloo, Waterloo, Canada
Jozef Tremko
Affiliation:
Skalnate Pleso Observatory, Tatranska Lomnica, Czechoslovakia

Abstract

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It has been found that the close spectroscopic pair of this system consists of a G type primary and a late type secondary, which most likely is a T Tauri star. As such, the system is semidetached and a mass transfer takes place between the components.

Type
Part I: Evolution of Stars in the Post-Main Sequence Stage
Information
International Astronomical Union Colloquium , Volume 69: Binary and Multiple Stars as Tracers of Stellar Evolution , 1982 , pp. 67 - 71
Copyright
Copyright © Reidel 1982

References

Batten, A.H., Morbey, C.L., Fekel, F.C. and Tomkin, J.: 1979, Publ. Astron. Soc. Pacific 91, 304.Google Scholar
Parsamian, E.S.: 1977, Flare Stars, Symposium Byurakan Obs., Ed. Mirzoyan, L.V., Yerevan.Google Scholar
Scarfe, C.C.,: 1977, Info. Bull. Var. Stars. Comm. 27 I.A.U., No. 1357.Google Scholar