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For 32 central stars of PNe we present their parameters interpolated amongthe new evolutionary sequences. The derived stellar final masses are confinedbetween 0.53 and 0.58 $M_\odot$ in good agreement with the peak in the whitedwarf mass distribution. Consequently, the inferred star formation history ofthe Galactic bulge is well restricted between 3 and 11 Gyr and is compatiblewith other published studies. The new evolutionary tracks proved a very good asa tool for analysis of late stages of stars life. The result provide acompelling confirmation of the accelerated post-AGB evolution.

Post-AGB evolution much faster than previously thought