Broadband Spectral Analysis of PKS 0528+134: A Report on Six Years of EGRET Observations
Author(s) -
R. Mukherjee,
M. Bottcher,
R. C. Hartman,
P. Sreekumar,
D. J. Thompson,
W. A. Mahoney,
T. Pursimo,
A. Sillanpaa,
L. O. Takalo
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/308057
Subject(s) - physics , lorentz factor , gamma ray , synchrotron radiation , egret , electron , astrophysics , synchrotron , photon , spectral line , radiation , jet (fluid) , lorentz transformation , astronomy , optics , nuclear physics , classical mechanics , thermodynamics
The multiwavelength spectra of PKS 0528+134 during six years of observationsby EGRET have been analyzed using synchrotron self-Compton (SSC) and externalradiation Compton (ERC) models. We find that a two-component model, in whichthe target photons are produced externally to the gamma-ray emitting region,but also including an SSC component, is required to suitably reproduce thespectral energy distributions of the source. Our analysis indicates that thereis a trend in the observed properties of PKS 0528+134, as the source goes froma gamma-ray low state to a flaring state. We observe that during the highergamma-ray states, the bulk Lorentz factor of the jet increases and the ERCcomponent dominates the high-energy emission. Our model calculations indicatethe trend that the energies of the electrons giving rise to the synchrotronpeak decreases, and the power-ratio of the gamma-ray and low energy spectralcomponents increases, as the source goes from a low to a high gamma-ray state.Comment: 36 pages, 13 figures, final version accepted for publication in ApJ; includes minor modification
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