  Only four globular cluster planetary nebulae (GCPN) are known so far in the
Milky Way. About 50 new globular clusters have been recently discovered towards
the Galactic bulge. We present a search for planetary nebulae within 3 arcmin
of the new globular clusters, revealing the identification of new candidate
GCPN. These possible associations are PN SB 2 with the GC Minni 06, PN
G354.9-02.8 with the GC Minni 11, PN G356.8-03.6 with the GC Minni 28, and PN
Pe 2-11 with the GC Minni 31. We discard PN H 2-14 located well within the
projected tidal radius of the new globular cluster FSR1758 because they have
different measured radial velocities. These are interesting objects that need
follow-up observations (especially radial velocities) in order to confirm
membership, and to measure their physical properties in detail. If confirmed,
this would double the total number of Galactic GCPN.

Solar and Stellar Astrophysics;Astrophysics of Galaxies