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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2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
FRIIs show lower cluster association rates than FRIs (30.6% vs 48.6% volume-limited; 32.6% vs 45.6% paired), with the gap widening at high luminosity, yet similar environments once inside clusters.
citing papers explorer
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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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Probing the environments of FRI and FRII radio galaxies in LoTSS DR2 with galaxy clusters
FRIIs show lower cluster association rates than FRIs (30.6% vs 48.6% volume-limited; 32.6% vs 45.6% paired), with the gap widening at high luminosity, yet similar environments once inside clusters.