Radio Properties of the $\gamma$-ray Emitting CSO Candidate 2234+282
  Most of the gamma-ray emitting active galactic nuclei (AGN) are blazars,
although there is still a small fraction of non-blazar AGN in the Fermi/LAT
catalog. Among these misaligned gamma-ray-emitting AGN, a few can be classified
as Compact Symmetric Objects (CSOs). In contrast to blazars in which gamma-ray
emission is generally thought to originate from highly beamed relativistic
jets, the source of gamma-ray emission in unbeamed CSOs remains an open
question. The rarity of the gamma-ray emitting CSOs is a mystery as well. Here
we present the radio properties of the gamma-ray CSO candidate 2234+282.
