The most plausible explanation of the cyclic period changes in close binaries: the case of the RS CVn-type binary WW Dra

Author: Liao W.-P.   Qian S.-B.  

Publisher: Oxford University Press

ISSN: 0035-8711

Source: Monthly Notices of the Royal Astronomical Society, Vol.405, Iss.3, 2010-07, pp. : 1930-1939

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Abstract