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Fig. 6

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Best-fitting Newtonian orbital solution for the binary HD 4552,BD+120090. Top left: the angle φ as a function of inclination. The red circle shows the selected value. Top right: the angle φ - φ0 as a function of eccentricity. The red circle shows the selected value. Bottom left: the black crosses show χR2+χΓ2D2$\chi^2_R+\chi^2_{\Gamma_{\rm 2D}}$ as a function of vrad/v = sin ψ sin i. The red cross shows the observed value of Vrad/Vtot and its error (see Table B.4). Bottom right: the black crosses show χR2+χΓ2D2$\chi^2_R+\chi^2_{\Gamma_{\rm 2D}}$ as a function of γ2D. The red cross shows the value of Γ2D and its error (see Table B.4).

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