The S(1), 4.5 μm, and 8.0 μm images of three systems of H₂ knots. Top row: HOD07 6 at 6^h7^m41.2^s, −6°11^{﹩\arcmin﹩}14^{﹩\arcsec﹩} is the center of symmetry of a string of emission knots. Bottom row: HOD07 8 at 6^h7^m43.7^s, −6°10^{﹩\arcmin﹩}46^{﹩\arcsec﹩} is the likely center of a single‐sided jet. HOD07 9 at 6^h7^m44.0^s, −6°11^{﹩\arcmin﹩}2^{﹩\arcsec﹩} is a star associated with H₂ emission and the likely source of a bow shock.