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Fig. 9

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Positions of the hot post-AGB stars in the log Teff − log g diagram. The blue lines denote the post-HB evolutionary tracks according to Dorman et al. (1993) with core mass of 0.49, 0.5, 0.51 and 0.53 M and the red line denote the zero-age horizontal branch (ZAHB). The black lines denote the post-AGB evolutionary tracks according to Blöcker (1995) for core stellar masses of 0.605, 0625, 0.696, 0.836, and 0.940 M and the green lines represent the post-AGB evolutionary tracks according to Schönberner (1983) for core stellar masses of 0.546 and 0.565 M. For comparison, we include some sdOB stars (blue stars and filled blue circles) of the samples of Heber (1986) and Ahmad & Jeffery (2003).

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