Structure of the inner jet of OJ 287 VLBA data at 15 GHz in a
  super-resolution mode
  In this work we show the results obtained from the VLBA data at 15 GHz of OJ
287 in the super-resolution mode. The data showed a jet configuration in the
form of "fork" where superluminal components emerge via stationary components
at the northwest and the southeast close to the core to form parallel
trajectories along the southwest direction in the plane of the sky. This agrees
with a source structure of an extended, broad morphology of OJ 287.
