We report observations of the J = 3 --> 2 and J = 2 --> 1 transitions of Si
O and CS, the J(k) = 3(k) --> 2(k) and J(k) = 2(k) --> 1(k) transitions of
CH3OH, and the J = 1 --> 0 transition of HCO+, made with Swedish-ESO Submil
limetre Telescope (SEST), toward the highly collimated bipolar outflow BHR
71. Broad wing emission was detected toward the outflow lobes in all the ob
served molecular lines. The shapes of the profiles are strikingly different
from molecule to molecule. For CS and HCO+ the emission from the outflowin
g gas appears as a weak broad feature superposed upon a strong narrow emiss
ion from the quiescent ambient gas. For CH,OH the intensity of the broad em
ission feature is considerably stronger than that of the narrow component,
whereas for SiO the broad feature completely dominates the emission spectra
. The spatial distribution of the integrated wing emission is considerably
extended and broadly similar in all the observed molecular transitions, sho
wing well-separated blueshifted and redshifted lobes with FWHM angular size
s of 2'.4 x 1'.3 and 2'.4 x 1'.4, respectively. We find that the abundance
of methanol and silicon monoxide in the outflow lobes is enhanced with resp
ect to that of the ambient cloud by factors of up to similar to 40 and 350,
respectively. The large enhancements of methanal and silicon monoxide in t
he outflow lobes are most likely due to the release from grains of ice mant
les and Si-bearing species via shocks produced by the interaction between t
he outflow and dense ambient gas. On the other hand, we find that the abund
ance of HCO+ in the outflowing gas is smaller than that in the ambient gas
by about a factor of 20, a decrease consistent with theoretical predictions
of shock models.