We present high-sensitivity near-IR images of a carbon-rich proto-planetary
nebula, AFGL 618, obtained with the Subaru Telescope. These images have re
vealed "bullets" and "horns" extending farther out from the edges of the pr
eviously known bipolar lobes. The spatial coincidence between these near-IR
microstructures and the optical collimated outflow structure, together wit
h the detection of shock-excited, forbidden IR lines of atomic species, str
ongly suggests that these bullets and horns represent the locations from wh
ich [Fe ii] IR lines arise. We have also discovered CO clumps moving at gre
ater than 200 km s(-1) at the positions of the near-IR bullets by reanalyzi
ng the existing (CO)-C-12 J = 1-0 interferometry data. These findings indic
ate that the near-IR microstructures represent the positions of shocked sur
faces at which fast-moving molecular clumps interface with the ambient circ
umstellar shell.