R. Morganti et al., BEPPOSAX OBSERVATIONS OF 2 JY LOBE-DOMINATED BROAD-LINE SOURCES - THEDISCOVERY OF A HARD X-RAY COMPONENT, Nuclear physics. B, Proceedings supplement, 69(1-3), 1999, pp. 435-438
We present new BeppoSAX LEGS, MECS, and PDS observations of five lobe-
dominated, broad-line active galactic nuclei selected from the 2 Jy sa
mple of southern radio sources. These include three radio quasars and
two broad-line radio galaxies. ROSAT PSPC data, available for all the
objects, are also used to Letter constrain the spectral shape in the s
oft X-ray band. The collected data cover the 0.1-10 keV energy range,
reaching 40 keV for one source. Detailed spectral fitting shows that a
ll sources have a flat hard X-ray spectrum with energy index alpha(x)
similar to 0.75 in the 2 - 10 keV energy range. This is a new result,
which is at variance with the situation at lower energies where these
sources exhibit steeper spectra. Spectral breaks similar to 0.5 at 1 -
2 keV characterize the overall X-ray spectra of our objects. The flat
, high-energy slope is very similar to that displayed by flat-spectrum
/core-dominated quasars, which suggests that the same emission mechani
sm (most likely inverse Compton) produces the hard X-ray spectra in bo
th classes. Contrary to the optical evidence for some of our sources,
no absorption above the Galactic value is found in our sample. Finally
, a (weak) thermal component is also present at low energies in the tw
o broad-line radio galaxies included in our study.