Fig. 9
Period–eccentricity distribution of different types of post-AGB binaries that have undergone a mass-loss phase in their past: dusty pAGB binaries (green squares, Waters et al. 1993; Van Winckel et al. 1995, 1998, 1999, 2000, 2009; Pollard et al. 1996; Gonzalez & Wallerstein 1996; Maas et al. 2002, 2005; Van Winckel 2007; Gorlova et al. 2014; Gezer et al. 2015; De Smedt et al. 2016; Manick et al. 2017), Ba stars (blue circles, Van der Swaelmen et al. 2017), Tc-poor S stars (black x’s, Van der Swaelmen et al. 2017) and the wide sdB binaries (red crosses, this article). See Sect. 6.2.
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