Rapid high-amplitude gamma-ray variability in Blazar PKS 0507+17
arXiv:1406.3834 · doi:10.1016/j.newast.2014.06.004
Abstract
We report a detailed analysis of -ray data of 2FGL J0509.9+1802 observed by the Large Area Telescope on board {\it Fermi} satellite, especially focusing on April 2013 when extraordinary -ray variability has been detected. Localization of -ray emission during this epoch suggests that the -ray source only associates with PKS 0507+17. The -ray emission of PKS 0507+17 is identified at the first time. The daily peak flux is over two orders of magnitude higher than the first two-year average flux, giving an isotropic -ray luminosity of erg . Rapid -ray variability with doubling time of 2-3 hours has been detected. Such a short doubling timescale has been detected for only a few bright blazars and indicates a location of -ray emission inside the broad line region. Together with the bluer-when-brighter -ray spectra, the variability phenomena could be well explained by the classic flat-spectrum radio quasar variability model that includes a fast injection of accelerated electrons and the external Compton cooling process.
arXiv commentAccepted for publication in New Astronomy
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