Right and center: P_I images at the H and K_s bands. Green contours indicate the position of the two stars. The two images are plotted in the same scale, using square root scaling. The pixels falling in the non-linear regime are set to zero. Left: the dotted and dashed lines indicate the position of large and micro jets, respectively (Whelan et al. 2010). Arrows “1”, “2”, and “3” indicate the polarized halo, the bright clump, and the sharp extended feature, respectively. Center: Arrows “a” and “d” show an artifact and a local decrement in polarized flux. The white line contours the Keck J-band image presented in Millan-Gabet & Monnier (2002). Right: relative polarized color computed as [H]−[K_s]. The white cross indicates the brightest point of feature “2” at the K_s band.