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Relativistic Jets in Low Power Radio Galaxies

  • G. Giovannini (a1) (a2), E. Arbizzani (a1), L. Feretti (a1), T. Venturi (a1), W.D. Cotton (a3), L. Lara (a4) and G.B. Taylor (a5)...

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 asymmetric 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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References

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Baum, S.A., et al. 1997. ApJ, 483 178193.
Feretti, L., et al. 1993. ApJ, 408, 446451.
Giovanmm, G., et al. 1990. ApJ, 358, 159163.
Giovanmm, G., et al. 1994. ApJ, 435, 116127.
Lara, L., et al. 1997a. ApJ, 474, 179187.
Lara, L., et al. 1997b. Vistas in Astronomy, 41, 241245.

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