  An H$_2$ emission filament is found in close proximity to the unique object
KH 15D using the adaptive optics system of the Subaru Telescope. The morphology
of the filament, the presence of spectroscopic outflow signatures observed by
Hamilton et al., and the detection of extended H$_2$ emission from KH 15D by
Deming, Charbonneau, & Harrington suggest that this filament arises from
shocked H$_2$ in an outflow. The filament extends about 15" to the north of KH
15D.
