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Z\\,CMa is a binary composed of an embedded Herbig Be and an FU Ori class star separated by $\\sim100$ au. Observational evidence indicate a complex environment in which each star has a circumstellar disk and drives a jet, and the whole system is embedded in a large dusty envelope.\n  Aims. We aim to probe the circumbinary environment of Z\\,CMa in the inner 400 au in scattered light.\n  Methods. We use high contrast imaging polarimetry with VLT/NaCo at $H$ and $K_s$ bands.\n  Results. The central binary is resolved in both bands. The polarized images show three bright and complex structure","authors_text":"C. Caceres, C. Dougados, F. M\\'enard, H. Canovas, J. de Boer, J.H. Girard, L.A. Cieza, M.R. Schreiber, S. Casassus, S. 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