Evolutional relationship between the γ-ray flares and millimeter wave outbursts in PKS 0528+134.

Astronomy and Astrophysics – Astrophysics

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Quasars: Outbursts, Quasars: Gamma Rays, Quasars: Mm Radiation, Quasars: Spectral Evolution

Scientific paper

During the period of 1991 - 1993 two strong high energy γ-ray flares were observed in the flat spectrum radio source PKS 0528+134. They were associated with strong mm-radio outbursts with a few months time-delays. In this paper the spectral energy distributions of the radiations in the γ-hard X-ray and the IR-optical bands are analysed. It is shown that the high energy γ-ray radiation may be due to the inverse Compton scattering of the ambient UV and soft X-ray photons by the relativistic electrons in the jet. Based on the comparison between the properties of the synchrotron radiation of the γ-ray source and the spectral evolution of the mm-radio outbursts, the evolutional relationship between the γ-ray emitting blobs and the mm-radio emitting blobs is discussed.

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