We have combined all OSSE spectra of the Orion molecular cloud complex
obtained through the end of 1996 and searched them for evidence of co
smic-ray induced gamma-ray lines in the 3-7 MeV energy range, as detec
ted by COMPTEL (Bloemen et al. 1994, 1997). We do not detect any signi
ficant line emission; our flux estimate for broad-line emission of 1.5
+/- 1.0 10(-4) gamma/(cm(2)-s) is consistent with the spatially-exten
ded flux 1.3 10(-4) gamma/(cm(2)-s) measured by Bloemen et al. (1997).