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Fig. 2

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Radial velocities of ASAS-09 (left) and ASAS-21 (right) from our AAT/UCLES (stars) and Radcliffe/GIRAFFE (squares) spectra together with the best fitting models. The measurements for the primaries are plotted with open and for the secondaries with filled symbols. The solid line shows the best fit for the primaries and the dashed line for the secondaries. The dotted line shows the systemic velocity γ.

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