  We present results from SMA observations of the star forming region Cepheus
A-East at ~340 GHz (875 micron) with 0.7'' - 2'' resolution. At least four
compact submm continuum sources have been detected, as well as a rich forest of
hot core line emission. Two kinematically, chemically, and thermally distinct
regions of molecular emission are present in the vicinity of the HW2 thermal
jet, both spatially distinct from the submm counterpart to HW2. We propose that
this emission is indicative of multiple protostars rather than a massive disk
as reported by Patel et al. (2005).
