A 2.12 μm S(1) line + continuum image containing three separate systems of H₂ knots. HOD07 4 at 6^h7^m35.3^s, −6°20^{﹩\arcmin﹩}0^{﹩\arcsec﹩} appears as a star with nebulous knots. As shown in Fig. 8, this position is most likely not the central source of this outflow. HOD07 5 at 6^h7^m38.7^s, −6°21^{﹩\arcmin﹩}14^{﹩\arcsec﹩} is the likely central star of this bipolar jet. HOD07 7 at 6^h7^m41.5^s, −6°21^{﹩\arcmin﹩}28^{﹩\arcsec﹩} is the likely position of the outflow center of that jet.