We have undertaken a deep investigation of a well defined sample of 136 PNe
located in a 10x10 degree central region of the Galactic Bulge observed with
the ESO VLT and supplemented by archival HST imagery. These studies have
provided precise morphologies, major axes position angles and the most robust
sample of consistently derived chemical abundances available to date. Using
these data we have statistically confirmed, at 5-sigma, the precise PNe
population that provides the PNe alignment of major axes previously suggested
in the Galactic Bulge, revealed a partial solution to the sulfur anomaly and
uncovered interesting morphological, abundance and kinematic features. We
summarise the most significant findings here with detailed results appearing in
a series of related publications.Comment: 6 pages, 5 figure