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- W4251840675 abstract "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." @default.
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- W4251840675 date "1982-01-01" @default.
- W4251840675 modified "2023-10-18" @default.
- W4251840675 title "The Age of the Triple System HD 165590" @default.
- W4251840675 cites W2030101138 @default.
- W4251840675 doi "https://doi.org/10.1017/s0252921100100363" @default.
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