  We investigate the X-ray properties of the most luminous radio sources in the
3CR catalogue, in order to assess if they are similar to the most luminous
radio quiet quasars, for instance in the X-ray normalization with respect to
the optical luminosity, or in the distribution of the absorption column
density. We have selected the (optically identified) 3CR radio sources whose
178-MHz monochromatic luminosity lies in the highest factor-of-three bin. The 4
most luminous objects had already been observed in X rays. Of the remaining 16,
we observed with XMM-Newton 4 randomly chosen, optical type 1s, and 4 type 2s.
All targets have been detected. The optical-to-Xray spectral index, alphaox,
can be computed only for the type 1s and, in agreement with previous studies,
is found to be flatter than in radio quiet quasars of similar luminosity.
However, the Compton thin type 2s have an absorption corrected X-ray luminosity
systematically lower than the type 1s, by a factor which makes them consistent
with the radio quiet alphaox. Within the limited statistics, the Compton thick
objects seem to have a reflected component more luminous than the Compton thin
ones. The extra X-ray component observed in type 1 radio loud quasars is beamed
for intrinsic causes, and is not collimated by the absorbing torus as is the
case for the (intrinsically isotropic) disk emission. The extra component can
be associated with a relativistic outflow, provided that the flow opening angle
and the Doppler beaming factor are 1/5 - 1/7 radians.
