Intra-cluster patches of baryons in the core of the Fornax cluster
E. Iodice, M. Spavone, M. Cantiello, R. DAbrusco, M. Capaccioli, M., Hilker, S. Mieske, N. Napolitano, R. Peletier, L. Limatola, A. Grado, A., Venhola, M. Paolillo, G. Van de Ven, P. Schipani

TL;DR
This study uncovers faint intra-cluster light patches in the Fornax cluster core, linking them to blue globular cluster over-densities and supporting a tidal stripping formation scenario in a dynamically evolved cluster.
Contribution
It reports the discovery of intra-cluster light patches in Fornax and correlates them with globular cluster over-densities, providing observational evidence for ICL formation via tidal stripping.
Findings
Detected faint intra-cluster light patches in Fornax core.
Found ICL luminosity is about 5% of NGC1399's total.
Supported tidal stripping as the ICL formation mechanism.
Abstract
In the core of the Fornax cluster, on the West side of NGC1399, we have detected a previously unknown region of intra-cluster light (ICL). It is made up by several faint (~mag/arcsec) {\it patches} of diffuse light. The bulk of the ICL is located in between the three bright galaxies in the core, NGC1387, NGC1379 and NGC1381, at ~arcmin (~kpc) from the central galaxy NGC~1399. We show that the ICL is the counterpart in the diffuse light of the known over-density in the population of blue globular clusters (GCs). The total g-band luminosity of the ICL is , which is of the total luminosity of NGC1399. This is consistent with the fraction of the blue GCs in the same region of the cluster. The ICL has ~mag, which is similar to the colors in the halo of the bright…
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