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The Age of the Triple System HD 165590
Published online by Cambridge University Press: 12 April 2016
Abstract
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
- Copyright
- Copyright © Reidel 1982