Intra-cluster GC-LMXB in the Fornax galaxy cluster. (arXiv:1909.06383v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Riccio_G/0/1/0/all/0/1">Gabriele Riccio</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Paolillo_M/0/1/0/all/0/1">Maurizio Paolillo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+DAbrusco_R/0/1/0/all/0/1">Raffaele D&#x27;Abrusco</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cantiello_M/0/1/0/all/0/1">Michele Cantiello</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jin_X/0/1/0/all/0/1">Xiangyu Jin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Li_Z/0/1/0/all/0/1">Zhiyuan Li</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Venhola_A/0/1/0/all/0/1">Aku Venhola</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+DAgo_G/0/1/0/all/0/1">Giuseppe D&#x27;Ago</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Puzia_T/0/1/0/all/0/1">Thomas Puzia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Iodice_E/0/1/0/all/0/1">Enrica Iodice</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pota_V/0/1/0/all/0/1">Vincenzo Pota</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Napolitano_N/0/1/0/all/0/1">Nicola Napolitano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hilker_M/0/1/0/all/0/1">Michael Hilker</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mieske_S/0/1/0/all/0/1">Steffen Mieske</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Spavone_M/0/1/0/all/0/1">Marilena Spavone</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Peletier_R/0/1/0/all/0/1">Reynier Peletier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Eigenthaler_P/0/1/0/all/0/1">Paul Eigenthaler</a>

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.

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.

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