The binary X-ray pulsar Her X-1 has been observed by CGRO-OSSE during
its Main-On state in July 1994. The average pulse period is determined
. Main-On pulse profiles in the 30-60 keV range for successive binary
orbits are compatible with a constant pulse width. A thin thermal brem
sstrahlung spectrum is fitted to the phase average data, yielding kT =
15(1) keV.