Fig. 6.
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Distance from Bailer-Jones et al. (2021) versus X-ray luminosity showing the position of the 213 period-bounce candidates (in color scale) and the eROSITA-detected confirmed period-bouncers (in triangles, bona fide period-bouncers are highlighted in black). The average eRASS:4 sensitivity limit is marked by the blue line (see text in Sect. 4). Black borders are used to show possible resolved binaries in the eROSITA WD subsample.
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