VLBI imaging at 4.9-43.2 GHz resolves symmetric parabolically expanding twin jets in 3C 452 to a few thousand Schwarzschild radii, with low Doppler factors indicating a viewing angle of about 70 degrees.
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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.
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The twin-jet system in the FRII radio galaxy 3C 452: A sub-parsec scale VLBI study
VLBI imaging at 4.9-43.2 GHz resolves symmetric parabolically expanding twin jets in 3C 452 to a few thousand Schwarzschild radii, with low Doppler factors indicating a viewing angle of about 70 degrees.
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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.