We have investigated the gas-phase chemistry in dense cores where ice
mantles containing ethanol and other alcohols have been evaporated. Mo
del calculations show that methanol, ethanol propanol, and butanol dri
ve a chemistry leading to the formation of several large ethers and es
ters. Of these molecules, methyl ethyl ether (CH3OC2H5) and diethyl et
her [(C2H5)(2)O] attain the highest abundances and should be present i
n detectable quantities within cores rich in ethanol and methanol. Gas
-phase reactions act to destroy evaporated ethanol and a low observed
abundance of gas-phase C2H5OH does not rule out a high solid-phase abu
ndance. Grain surface formation mechanisms and other possible gas-phas
e reactions driven by alcohols are discussed, as are observing strateg
ies for the detection of these large interstellar molecules.