The origin of jets and hot spots in FR II double radio sources are explaine
d by a model in which a supermassive black hole possessing twin beams moves
out of the host galaxy with a speed greater than the escape speed. The lob
e structure arises as a combination of two trails: the trail of the forward
pointing beam is the lobe itself while the backward-pointing beam creates
the so-called "jet" (narrow linear high-brightness feature). We show that t
he formation of the "jet" depends on the beam angle relative to the line of
motion of the black hole. The same angle also controls the amount of entra
inment of thermal gas in the lobe, and correlations between the component d
epolarization and the existence of a jet may arise through this common fact
or. The high-resolution samples of FR II radio galaxies at z < 0.3 by Hardc
astle et al. and a representative sample of radio quasars by Bridle et al.
are studied for evidence of the beam angle correlation with the jet formati
on.