We propose to use CAM+CVF to carry out an independent
search for outflows in a list of IRAS sources in Bok globules.
By observing in the 9.66 micron 0-0 S(3) line of H2, we will
be sensitive to low velocity shocks which should be plentiful
in the outflow environment. We believe this technique has
greater sensitivity than mm outflow searches, and by observing
IRAS sources with a range of spectral indices will be able to
test the idea that outflows cease in going from steep to
shallow spectrum (more evolved) objects.