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- W2017908808 abstract "During the period of 1991–1993 two strong high energy γ-ray flares were observed by the Compton Gamma Ray Observatory 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 (SED) of the radiations in the γ-hand 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. Basing 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." @default.
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- W2017908808 date "1998-10-01" @default.
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- W2017908808 title "Evolutionary relationship between the γ-ray flares and millimeter wave outbursts in PKS 0528+134" @default.
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- W2017908808 doi "https://doi.org/10.1016/s0275-1062(98)00052-6" @default.
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