  We report the negative results of our searches in COMPTEL data for 1.809 MeV
gamma-ray line emission from four localized regions which contain nearby
supernova remnants (SNRs). The upper flux limits (2 Sigma) are found to be in
the range of 1.4*10e-5 to 2.4*10e-5 photons/s/cm/cm. These upper limits do not
severely constrain the theoretical 26Al yields from individual core collapse
supernovae due to large uncertainties in the SNR distances and the nature of
the progenitor stars.
