  Thanks to SAURON integral-field observations we uncovered the Planetary
Nebulae (PNe) populations inhabiting the central and nuclear regions of our
galactic neighbours M32 and M31, respectively, and discuss the significant
differences between their corresponding PNe luminosity functions in light of
the properties of their parent stellar populations. In particular, we conclude
that the lack of bright PNe in the nuclear regions of M31 is likely linked to
the nearly Solar value for the stellar metallicity, consistent with previous
suggestions that a larger metallicity would bias the Horizontal-Branch (HB)
populations toward bluer colors, with fewer red HB stars capable of producing
PNe and more blue HB stars that instead could contribute to the far-UV flux
that is observed in metal-rich early-type galaxies and, incidentally, also in
the nucleus of M31.
