Testing gravity with wide binaries - 3D velocities and distances of wide binaries from Gaia and HARPS

Open Access

Fig. 16

Correlations with Γ_2D (left) and Γ_3D (right). The top plots show both angles as a function of inclination, circled WBs have eccentricities larger than 0.8. The bottom plots show both angles as function of orbit phase, circled WBs have inclinations larger than 70°.

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