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Synchrotron Self‐Compton Model for Rapid Nonthermal Flares in Blazars with Frequency‐dependent Time Lags

  • Sokolov A
  • Marscher A
  • McHardy I
The Astrophysical Journal (2004) 613(2) 725-746
DOI: 10.1086/423165
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Abstract

inverse Compton scatteringmultifrequency emission from blazarsvariabilityX-raysWe show that the pronounced negative time delay between the X-rayand IR light curves (X-rays peak after the maximum in the synchrotronemission) can be accounted for if both forward and reverse shocksare considered.

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Sokolov, A., Marscher, A. P., & McHardy, I. M. (2004). Synchrotron Self‐Compton Model for Rapid Nonthermal Flares in Blazars with Frequency‐dependent Time Lags. The Astrophysical Journal, 613(2), 725–746. https://doi.org/10.1086/423165

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