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A possible relation between the period change and the mass ratio for W-type contact binaries
Authors:Shengbang Qian
Affiliation:1Yunnan Observatory, Chinese Academy of Sciences, PO Box 110, 650011 Kunming, China;2National Astronomical Observatories, Chinese Academy of Sciences (NAOCAS), 100012 Beijing, China;3 United Laboratory of Optical Astronomy, Chinese Academy of Sciences (ULOAC), 100012 Beijing, China
Abstract:
Keywords:binaries: close    stars: evolution    stars: general
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