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- W33255199 abstract "New photometric data from the eclipsing binary star AI Draconis has been analyzed with the method of WilsonDevinney. The system shows a period increase of about 0.91 sec per century, which corresponds to a mass transfer from the less to the more massive component at a rate of 7.5 10 M /yr under the conservative mass transfer hypothesis. We also suggest that the system has an unseen component which orbits around the mass center of the triplet system with a period of about 23 yrs. We found that the projectional angular separation between the third star and eclipsing pair varies from 0. 048 to 0. 235. These results suggestive of a third body should be checked in the future with more sensitive observations." @default.
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- W33255199 date "2000-11-01" @default.
- W33255199 modified "2023-10-18" @default.
- W33255199 title "Photometric analysis of the eclipsing binary star AI Draconis" @default.
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