G. Giovannini et al., VLBI OBSERVATIONS OF A COMPLETE SAMPLE OF RADIO GALAXIES .4. THE RADIO GALAXIES NGC-2484, 3C-109, AND 3C-382, The Astrophysical journal, 435(1), 1994, pp. 116-127
We present here new VLBI observations of one F-R I radio galaxy (NGC 2
484) and two broad-line F-R II radio galaxies (3C 109 and 3C 382). For
3C 109 new VLA maps are also shown. These sources belong to a complet
e sample of radio galaxies under study for a better knowledge of their
structures at parsec resolution. The parsec structure of these three
objects is very similar: asymmetric emission, which we interpret as th
e core plus a one-sided jet. The parsec-scale jet is always on the sam
e side of the main kiloparsec-scale jet. The limit on the jet to count
erjet brightness ratio, the ratio of the core radio power to the total
radio power and the synchrotron-self Compton model allow us to derive
some constraints on the jet velocity and orientation with respect to
the line of sight. From these data and from those published on two oth
er sources of our sample, we suggest that parsec-scale jets are relati
vistic in both F-R I and F-R II radio galaxies and that parsec scale p
roperties in F-R I and F-R II radio galaxies are very similar despite
the large difference between these two classes of radio galaxies on th
e kiloparsec scale.