Fig. 10.
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Extinction-corrected Hertzsprung-Russell (HR) diagram. All Gaia sources within 100 pc with significantly measured parallaxes (parallax_over_error > 3) are shown in gray (Gaia Collaboration 2023). The star markers represent new spectroscopically confirmed CVs (blue) and variable CV candidates (white) from Table 1. The white circles indicate CV candidates selected by a FX/Fopt ratio and Gaia (BP–RP) color: (1) J165219.0–441401; (2) J173332.5–181735; (3) J094607.7–311550; (4) J155926.5–754311; (5) J190823.2+343328; (6) J173555.3–292530.
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