Model-subtracted WIDE-S image of U Hya (see text) shown in the equatorial coordinates. North is up and east to the left. The axes give the offsets with respect the star. Pixel size is 15″. The subtracted model is the one with α =  −4.5 in Table 4, arbitrarily multiplied by 0.85 so that the extended components become the most evident. Excess emission (“1”) is seen to the east of the shell along PA ~  −70° with respect to the star in the equatorial coordinates. Its peak brightness is  ~4 MJy sr^-1 above the background level. Other excesses at PA ~  −7°(“2”) and  ~180°(“3”) from circular symmetry in the shell brightness distribution is also discernible (see text).