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Fig. 11

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Fill black circles and open circles are UVES radial velocity measurements of the primary and secondary components of the 45368 binary system. The solid curve is the best-fitting model in phase with the primary eclipses. The dotted line is the best-fitting model in phase with the secondary eclipse. The dashed horizontal line indicates the baricentric velocity of the system (γ =  −30.19   km   s-1).

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