Jet propagation along a triaxial galaxy's major axis produces X-shaped radio morphologies while minor-axis alignment yields classical double-lobed sources, with intermediate angles creating regenerative boomerang structures.
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Observational VLBI study of parsec-scale jets in 15 gamma-ray radio galaxies finds core flux density correlates with gamma-ray flux but gamma-ray luminosity shows no dependence on brightness temperature or core dominance.
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Galactic-scale evolution of classical and complex radio galaxies. Impact of ambient morphology and jet geometry
Jet propagation along a triaxial galaxy's major axis produces X-shaped radio morphologies while minor-axis alignment yields classical double-lobed sources, with intermediate angles creating regenerative boomerang structures.
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Gamma-ray emission in radio galaxies under the VLBI scope -- I. Parsec-scale kinematics and high-energy properties of $\gamma$-ray detected TANAMI radio galaxies
Observational VLBI study of parsec-scale jets in 15 gamma-ray radio galaxies finds core flux density correlates with gamma-ray flux but gamma-ray luminosity shows no dependence on brightness temperature or core dominance.