GRS 1915+105 was observed by the Oriented Scintillation Spectroscopy Experi
ment (OSSE) aboard the Compton Gamma Ray Observatory nine times in 1995-200
0, and eight of those observations were simultaneous with those by the Ross
i X-Ray Timing Explorer (RXTE). We present an analysis of all of the OSSE d
ata and of two RXTE-OSSE spectra with the lowest and highest X-ray fluxes.
The OSSE data show a power-law-like spectrum extending up to greater than o
r similar to 600 keV without any break. We interpret this emission as stron
g evidence for the presence of nonthermal electrons in the source. The broa
dband spectra cannot be described by either thermal or bulk-motion Comptoni
zation, whereas they are well described by Comptonization in hybrid thermal
/nonthermal plasmas.