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Monthly Notices of the Royal Astronomical Society 367 (1) 423 (2006)
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The most plausible explanation of the cyclic period changes in close binaries: the case of the RS CVn-type binary WW Dra

W.-P. Liao and S.-B. Qian
Monthly Notices of the Royal Astronomical Society no (2010)
DOI: 10.1111/j.1365-2966.2010.16584.x
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