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- W1526062280 abstract "The UBV observations of the close binary system CW Cephei were made from August 198:3 to December 1984 during 25 nights using the 61cm Boller and Chivens reflector at the Sobaeksan Astronomy Observatory. The new UBV light curves were analyzed with the recent Wilson-Devinney binary model. Our photometric solution for CW Cep were well consistent with those of Clausen &. Gimenez (1991). Using our photometric solution and Popper & Hill (1991) spectroscopic one, each absolute masses and radii of components for CW Cep were derived as 13.63 M and 5.83 R for the primary, and 12.18 M and 5.14 R for the secondary, respectively." @default.
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- W1526062280 date "1996-12-01" @default.
- W1526062280 modified "2023-10-17" @default.
- W1526062280 title "LIGHT CURVE ANALYSIS OF CW CEPHEI" @default.
- W1526062280 hasPublicationYear "1996" @default.
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