  We show that the 4.44 and 6.13 MeV line emission observed with COMPTEL from
Orion is consistent with gamma ray spectra consisting of a mixture of narrow
and broad lines or spectra containing only broad lines. We employed several
accelerated particle compositions and showed that the current COMPTEL data in
the 3--7 MeV region alone cannot distinguish between the various possibilities.
However, the COMPTEL upper limits in the 1--3 MeV band favor a composition
similar to that of the winds of Wolf-Rayet stars of spectral type WC. The power
dissipated by the accelerated particles at Orion is about 4 $\times$ 10$^{38}$
erg s$^{-1}$. These particles are not expected to produce significant amounts
of $^{26}$Al.
