THE HIGH-ENERGY CONTINUUM EMISSION OF THE GAMMA-RAY BLAZAR PKS-0528+134

We present Advanced Satellite for Cosmology and Astrophysics (ASCA) ob servations of the gamma-ray blazar PKS 0528 + 134, obtained at two sep arate epochs in 1994 August and 1995 March. These data represent the f irst measurement of the X-ray continuum emission of this source in the medium-hard X-ray band. Both ASCA spectra are consistent with a singl e power law with photon index Gamma similar to 1.7-1.8 and column dens ity N-H similar to 5 x 10(21) cm(-2), higher than Galactic. The X-ray flux increased by a factor of 4 in similar to 7 months without appreci able change of the spectral shape. During the lower state of 1994 Augu st, PKS 0528 + 134 was observed simultaneously in the optical, X-rays, . and at gamma-ray energies with EGRET. The gamma-ray intensity is the faintest detected thus far in the source, with a steep spectrum (Gamm a similar to 2.7). The extrapolation of the X-ray continuum to the gam ma-ray range requires a sharp spectral break at similar to 10(22) Hz. We discuss the radio through gamma-ray spectral energy distribution of PKS 0528 + 134, comparing the low state of 1994 August with the flare state of 1993 March. We show that in PKS 0528+134, a nonnegligible co ntribution from the external radiation held is present and that, altho ugh synchrotron self-Compton scenarios cannot be ruled out, inverse Co mpton upscattering of thermal seed photons may be the dominant cooling process for the production of the high-energy continuum in this blaza r.