  A millimeter molecular line survey of three carbon-rich AGB stars and two
oxygen-rich planetary nebulae has been carried out over the frequency range
80.5-115.5 GHz. Sixty eight different transitions were detected in the data
from 27 different molecular species. The hyperfine structure of C2H and C13CH
has been fitted to constrain the optical depth of their transitions. All other
transitions have been constrained on the basis of their line profile shapes.
Rotation temperatures and column densities have been calculated for all
possible species, with adaptations to the methods applied in order to account
for the hyperfine structure of various transitions. From the column densities,
carbon, silicon and sulphur isotopic ratios have been determined. The results
corroborate IRAS 15194-5115 as a J-type star, whilst excluding IRAS 15082-4808
and IRAS 07454-7112 as such.
