  We present the results of a multi-faceted study of the high-mass star-forming
region S235. With the CalTech Submillimeter Observatory (CSO), we have observed
and/or mapped over fifty molecular transitions and 350 micron dust emission in
an attempt to learn more about the chemistry, kinematics, and mass distribution
within this rich region. We have found two dust cores that are not resolved in
our molecular line observations and suggest that one of these is a less evolved
star-forming core.
