  Since its launch INTEGRAL has devoted a significant fraction of its observing
time to the Galactic plane region. We present the results of INTEGRAL
observations of the inner spiral arms of the Galaxy (Norma, Scutum and
Sagittarius) with attention to high mass X-ray binaries. The increased
sensitivity of the survey and possibility to detect absorbed sources
significantly enlarged our sample of HMXBs in comparison with previous studies.
For some absorbed sources we present for the first time high quality broadband
(1-100 keV) energy spectra. We confirm pulsations of the X-ray flux of IGR
J16358-4726, discovered by CHANDRA, and report discovery of pulsations with a
period of $228\pm6$ sec from IGR J16465-4507. We confirm that the Galactic high
mass X-ray binary distribution is significantly different from the distribution
of low mass X-ray binaries concentrated in the Galactic Center. A large
fraction of detected high mass X-ray binaries are absorbed sources.
