An accelerating plasma blob crossing the BLR in 3C 279 reproduces the 2013 orphan gamma-ray flare's hard spectrum, rapid rise, slow decay, and lack of optical variability via varying external Compton scattering.
author Diltz , C
3 Pith papers cite this work, alongside 35 external citations. Polarity classification is still indexing.
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A 14-year, 168-epoch SED study of 3C 279 finds that a one-zone leptonic model with varying Doppler factor and electron population can explain the flares, with the emission region outside the BLR in most states.
Multi-wavelength monitoring of a gamma-ray flare in 1H 0323+342 reveals sub-hour variability, jet-corona transition, and ~10^46 erg/s jet power via external Compton modeling of disk and BLR photons.
citing papers explorer
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Blazar flares from plasma blobs crossing the broad-line region
An accelerating plasma blob crossing the BLR in 3C 279 reproduces the 2013 orphan gamma-ray flare's hard spectrum, rapid rise, slow decay, and lack of optical variability via varying external Compton scattering.
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Modeling the Multiwavelength Emission of 3C 279 during the 14 years of Fermi-LAT Era
A 14-year, 168-epoch SED study of 3C 279 finds that a one-zone leptonic model with varying Doppler factor and electron population can explain the flares, with the emission region outside the BLR in most states.
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A Rare Gamma-ray Flaring episode of the Narrow-Line Seyfert 1 Galaxy 1H 0323+342
Multi-wavelength monitoring of a gamma-ray flare in 1H 0323+342 reveals sub-hour variability, jet-corona transition, and ~10^46 erg/s jet power via external Compton modeling of disk and BLR photons.