Fig. A.6.
Position of LS V+22 25 (blue error bars) in the (Teff, log(g)) diagram: the black solid lines are pre-He-WD tracks from Driebe et al. (1998) labeled with their respective masses. The position of HZ 22 (red error bars; Shimanskii 2002), evolutionary tracks for nonrotating stars of solar metallicity (gray dashed lines; Ekström et al. 2012), and the corresponding ZAMS are shown for reference.
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