  BeppoSAX observations of the Seyfert galaxies Mrk 509 and MCG+8-11-11 are
presented. Earlier evidence of a soft excess in Mrk 509 is confirmed. This
excess is found to be better represented by a power law than by a black body:
with a photon slope of 2.5, its extrapolation matches the flux recorded in the
far UV. An ASCA observation, which appeared to exclude the presence of the
excess while showing instead evidence of a warm absorber, turns out to be
compatible with the coexistence of the excess seen with BeppoSAX and of the
warm absorber. The hard power law of Mrk 509 is seen for the first time to be
affected by a cut-off at high energies, with an e-folding energy of about 70
keV. In MCG+8-11-11 the cut-off is found at about 170 keV, consistent within
the combined errors with a previous estimate from a ASCA+OSSE/CGRO observation.
In both objects the reflection component is clearly detected. In Mrk 509 its
strength, together with that of the iron K line, indicates a solid angle Omega,
subtended by the reprocessing gas in the accretion disk, much less than 2pi,
but lacking a valid constraint on the inclination angle this evidence is not as
convincing as that found with BeppoSAX in IC 4329A. In MCG+8-11-11 the same
parameters are instead consistent with Omega=2pi, but the comparison with an
ASCA observation, when the flux level was about 2.5 times weaker, suggests that
a substantial fraction of the angle might be associated with gas farther out
than the accretion disk.
