Fig. 3.
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Comparison of the separations between the optical and Xray source of the Gaia DR3 WD from Gentile Fusillo et al. (2021) versus the companion in a possible resolved binary. The angular separation between the components of the possible resolved binary is shown as a color scale. We highlight with black circles the known WD-MS wide binaries and with black triangles the WD-WD wide binaries (El-Badry & Rix 2018).
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