The 2.12 μm S(1), 4.5 μm, and 8.0 μm images of the three systems of H₂ knots found in the area of Fig. 7. The driving source of HOD07 4 is probably located at 6^h7^m37.6^s, −6°19^{﹩\arcmin﹩}54^{﹩\arcsec﹩}, marked by a very faint star and the apex of the jetlike nebulosity of the Spitzer 4.5 μm image. HOD07 5 lies at 6^h7^m38.7^s, −6°21^{﹩\arcmin﹩}14^{﹩\arcsec﹩}, identified by a faint source at the approximate center of symmetry of the bipolar jet. HOD07 7 at 6^h7^m41.5^s, −6°21^{﹩\arcmin﹩}28^{﹩\arcsec﹩} is the likely position of the driving source of a bipolar jet.