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Application of a new non-linear least squares velocity curve analysis technique for spectroscopic binary stars

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Velocity curve analysis of the spectroscopic binary stars RZ Cas, CC Cas, HS Her, HD 93917, V921 Her and Y Cygni by the artificial neural networks

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Synchronization and circularization in early-type binaries on main sequence

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Monthly Notices of the Royal Astronomical Society 401 (1) 257 (2010)
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Close binary systems in multiple stars: III. Eclipsing variables with LITE effect

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