Fig. 2
RVs of the centre of gravity of the eclipsing binary (red triangles) and component B (blue triangles) against the best-fitting model (black) corresponding to parameters listed in Table 5. ΔAa,Ab (in km s-1) denote residuals of the fit for RVs of the centre of gravity of the eclipsing binary, and ΔB (in km s-1) residuals of the fit for RVs of component B.
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