We present new molecular spectral line and (sub)millimetre continuum o
bservations of the IRAS2 region of NGC1333. Our data locates the (sub)
millimetre counterpart of the IRAS source. This source is located at t
he centre of symmetry of two bipolar molecular outflows. The older 'fo
ssil' outflow extends approximately north-south while a younger, highl
y collimated, jet-like east-west outflow terminates in a well-defined
molecular bow shock. Multi-transition methanol line data suggest that
the molecular bow shock is very cold and that shock interactions have
greatly enhanced the methanol abundance. This source provides a striki
ng example of a molecular counterpart to the frequently observed optic
al Herbig-Haro type bow shock structures and provides a valuable speci
men for detailed shock chemistry studies.