Why do only some Radio Galaxies acquire giant Sizes?
  We study the morphology of the radio emission of giant radio galaxies (GRGs),
a rare type of active galaxies, in order to find new clues for the reasons of
their large size. Using radio images from two sky surveys at 1.4 GHz we
quantified their radio morphology by measuring the geometry (armlength, bending
angle, etc.) and flux symmetry for 58 such objects. Preliminary analysis
suggests that radio source symmetry does not differ between galaxies and
quasars, that there is no evidence for a decrease in linear size with redshift,
and only a marginal trend for increasing symmetry with larger size. A merging
with data available for other such objects is expected to yield new clues on
the possible reasons for their large size. We also searched radio survey images
around the positions of 1059 galaxies and quasars for further giant radio
sources, and present a preliminary sample of six of these.
