Minniti, DanteDias, BrunoGómez, MatíasPalma, TaliPullen, Joyce B.2021-11-152021-11-152019-11Astrophysical Journal Letters Volume 884, Issue 110 October 2019 Article number L152041-8205http://repositorio.unab.cl/xmlui/handle/ria/20900Indexación: ScopusOnly four globular cluster planetary nebulae (GCPN) are known so far in the Milky Way. About 50 new globular clusters have been recently discovered toward the Galactic bulge. We present a search for planetary nebulae within 3′ 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. © 2019. The American Astronomical Society. All rights reserved..enPlanetary NebulaeStellar EvolutionWhite DwarfsArtículoAtribución 3.0 Chile (CC BY 3.0 CL)10.3847/2041-8213/ab4424