  We report the results from an ASCA X-ray observation of the powerful Broad
Line Radio Galaxy, 3C109. The ASCA spectra confirm our earlier ROSAT detection
of intrinsic X-ray absorption associated with the source. The absorbing
material obscures a central engine of quasar-like luminosity. The luminosity is
variable, having dropped by a factor of two since the ROSAT observations 4
years before. The ASCA data also provide evidence for a broad iron emission
line from the source, with an intrinsic FWHM of ~ 120,000 km/s. Interpreting
the line as fluorescent emission from the inner parts of an accretion disk, we
can constrain the inclination of the disk to be $> 35$ degree, and the inner
radius of the disk to be $< 70$ Schwarzschild radii. Our results support
unified schemes for active galaxies, and demonstrate a remarkable similarity
between the X-ray properties of this powerful radio source, and those of lower
luminosity, Seyfert 1 galaxies.
