  The formation of Low mass X-ray binaries (LMXB) is favored within dense
stellar systems such as Globular Clusters (GCs). The connection between LMXB
and Globular Clusters has been extensively studied in the literature, but these
studies have always been restricted to the innermost regions of galaxies. We
present a study of LMXB in GCs within the central 1.5 deg^2 of the Fornax
cluster with the aim of confirming the existence of a population of LMXB in
intra-cluster GCs and understand if their properties are related to the host
GCs, to the environment or/and to different formation channels.
