Fig. 9

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Location in the HR Diagram of the 118 post-AGB candidates with luminosities and temperatures derived using VOSA. Evolutionary tracks by Miller Bertolami (2016) are shown and the objects are colour-coded according to the classification shown in the legend. The upper panel shows those objects located within the Galactic disc, with |z| ≤ 1.25 kpc, and Z = 0.02 evolutionary tracks for comparison, while in the lower panel, those with |z| > 1.25 kpc (Galactic halo) together with Z = 0.001 tracks are shown.
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