BeppoSAX OBSERVATIONS OF SYNCHROTRON X–RAY EMISSION FROM RADIO QUASARS

We present new BeppoSAX LECS, MECS, and PDS observations of four flat–spectrum radio quasars (FSRQ) having effective spectral indices αro and αox typical of high-energy peaked BL Lacs. Our sources have X–ray–to–radio flux ratios on average ∼ 70 times larger than “classical” FSRQ and lie at the extreme end of the FSRQ X–ray–to–radio flux ratio distribution. The collected data cover the energy range 0.1− 10 keV (observer’s frame), reaching ∼ 100 keV for one object. The BeppoSAX band in one of our sources, RGB J1629+4008, is dominated by synchrotron emission peaking at ∼ 2 × 10 Hz, as also shown by its steep (energy index αx ∼ 1.5) spectrum. This makes this object the first known FSRQ whose X–ray emission is not due to inverse Compton radiation. Two other sources display a flat BeppoSAX spectrum (αx ∼ 0.7), with weak indications of steepening at low X–ray energies. The combination of BeppoSAX and ROSAT observations, (non-simultaneous) multifrequency data, and a synchrotron inverse Compton model suggest synchrotron peak frequencies ≈ 10 Hz, although a better coverage of their spectral energy distributions is needed to provide firmer values. If confirmed, these values would be typical of “intermediate” BL Lacs for which the synchrotron and inverse Compton components overlap in the BeppoSAX band. Our sources, although firmly in the radio–loud regime, have powers more typical of high–energy peaked BL Lacs than of FSRQ, and indeed their radio powers put them near the low–luminosity end of the FSRQ luminosity function. We discuss this in terms of an anti-correlation between synchrotron peak frequency and total power, based on physical arguments, and also as possibly due to a selection effect. Subject headings: radiation mechanisms: non-thermal—galaxies: active, quasars—X-rays: galaxies