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 .