A propagating jet disturbance in 3C 120 produces an orphan gamma-ray flare by inverse-Compton scattering synchrotron photons from a stationary feature at about 10 times the broad-line region radius.
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4 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 4representative citing papers
A tenfold larger sample of AGN radio source sizes confirms a real angular size-redshift relation but indicates that scatter must drop below 20% or samples reach thousands to 100,000 to constrain Ω_m effectively.
Fermi-LAT variability analysis of jetted AGNs finds mean damping timescales of ~100 days, greater amplitudes in FSRQs than BL Lacs, emission regions at 2-4.5 R_DT but 123-295 R_BLR, and correlations with luminosities, loudness, black hole mass, and Eddington ratio.
Correlations link the radio cores and select jet components in 3C 454.3 to portions of the observed gamma-ray variability, indicating multiple emission regions and synchrotron self-Compton processes.
citing papers explorer
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A Ring of Fire Orphan {\gamma}-Ray Flare in the Neutrino Candidate 3C 120
A propagating jet disturbance in 3C 120 produces an orphan gamma-ray flare by inverse-Compton scattering synchrotron photons from a stationary feature at about 10 times the broad-line region radius.
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Revisiting the angular size-redshift cosmological test with milliarcsecond radio structures in active galactic nuclei
A tenfold larger sample of AGN radio source sizes confirms a real angular size-redshift relation but indicates that scatter must drop below 20% or samples reach thousands to 100,000 to constrain Ω_m effectively.
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Characterizing the origins of gamma-ray variability of the jetted active galactic nuclei observed with the Fermi-LAT
Fermi-LAT variability analysis of jetted AGNs finds mean damping timescales of ~100 days, greater amplitudes in FSRQs than BL Lacs, emission regions at 2-4.5 R_DT but 123-295 R_BLR, and correlations with luminosities, loudness, black hole mass, and Eddington ratio.
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Relationship between the $\gamma-$ray variability and the pc-scale jet in the blazar 3C 454.3
Correlations link the radio cores and select jet components in 3C 454.3 to portions of the observed gamma-ray variability, indicating multiple emission regions and synchrotron self-Compton processes.