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