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- W1568898803 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.
- W1568898803 created "2016-06-24" @default.
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- W1568898803 date "1982-01-01" @default.
- W1568898803 modified "2023-09-23" @default.
- W1568898803 title "The Age of the Triple System HD 165590" @default.
- W1568898803 cites W2030101138 @default.
- W1568898803 doi "https://doi.org/10.1007/978-94-009-7861-4_9" @default.
- W1568898803 hasPublicationYear "1982" @default.
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