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

Open Access

Fig. 10

Residuals ΔV_rad/V_tot (left), ΔΓ_2D (middle), and ΔΓ_3D) (right) as a function of acceleration. We circle WBs with inclinations larger than 70° in the left, WBs with eccentricities larger than 0.8 in the middle, and WBs with r/a < 0.5 in the right plot.

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