We are using the new IRAS Sky Survey Atlas to construct a catalog of G
alactic dark clouds and their associated Young Stellar Objects (YSOs).
From IRAS 100 and 60 mu m data we calculate images of the 100 mu m op
tical depth distribution in the clouds. Using the IRAS Faint Source Ca
talog we identify sources which have colors indicative of YSOs and hav
e positions that lie inside cloud boundaries in the optical depth imag
es. Here we present some preliminary results of applying this analysis
to the Chamaeleon dark cloud complex.