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Paper: Relativistic Jets in Low Power Radio Galaxies
Volume: 144, Radio Emission from Galactic and Extragalactic Compact Sources, IAU Colloquium 164
Page: 85
Authors: Giovannini, G.; Arbizzani, E.; Feretti, L.; Venturi, T.; Cotton, W. D.; Lara, L.; Taylor, G. B.
Abstract: From VLBI observations of 11 FR I radio galaxies we find that: 1. parsec scale jets are relativistic; 2. 3C 264 shows a relativistic jet decelerating moving from the core to the extended lobes; 3. 3C 338} is a source with a symmetric parsec scale structure and morphological changes, implying proper motion on both sides of the source; 4. 1144+35 is an extended low power radio galaxy with an apparent superluminal motion in its parsec scale radio structure.
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