Clues on High Energy Emission Mechanism from Blazar 3C 454.3 during 2015 August Flare
arXiv:1705.06185 · doi:10.1093/mnras/stx1194
Abstract
We perform a detailed spectral study of a recent flaring activity from the Flat Spectrum Radio Quasar (FSRQ), 3C\,454.3, observed simultaneously in optical, UV, X-ray and -ray energies during 16 to 28 August, 2015. The source reached its peak -ray flux of on 22 August. The time averaged broadband spectral energy distribution (SED) is obtained for three time periods, namely "flaring state"; covering the peak -ray flux, "post flaring state"; immediately following the peak flare and "quiescent state"; separated from the flaring event and following the post flaring state. The SED corresponding to the flaring state is investigated using different emission models involving synchrotron, synchrotron self Compton (SSC) and external Compton (EC) mechanisms. Our study suggests that the X-ray and -ray emission from 3C\,454.3 cannot be attributed to a single emission mechanism and instead, one needs to consider both SSC and EC mechanisms. Moreover, the target photon energy responsible for the EC process corresponds to an equivalent temperature of 564 K, suggesting that the flare location lies beyond the broad line emitting region of the FSRQ. SED fitting of the other two flux states further supports these inferences.
28 pages, 9 figures, 5 tables Accepted 2017 May 12. Received 2017 May 12; in original form 2016 November 07
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- Localizing the -ray emitting region in the blazar TXS 2013+370
- Understanding the X-ray spectral curvature of Mkn 421 using broadband AstroSat observations
- On the origin of GeV spectral break for Fermi blazars: 3C 454.3
- Correlations between -ray luminosity and magnetization of the jet as well as relativistic electron injection power:cases for Mrk 421, 3C 454.3 and 3C 279