Abstract
0528 + 134 is flat-spectrum radio-loud Quasar with variable radio radiation with rapid structural changes in its physics' core. It has been regularly observed for more 22 years. In this paper, we present the comparison between the parameters approach of RDV (Research and Development) and those of MOJAVE (Monitoring of Jets in Active Galactic Nuclei with VLBA Experiments) and VLBA-BU-Blazar data. Moreover, we also introduce the multi-epoch images at 2.3 GHz, 8.15 GHz, 15.3 GHz and 43 GHz. Meanwhile, in the paper, there are the morphology and kinematics relating to the jet in the light of the prominence of this source in the physics regime. We can associate the increased activity in the S-band X-band, K-band and Q-band with morphological changes in the source structure and their relationship. In terms of applying our approach to the flux density limited sample of radio loud of physics objects, it is implied that AGN jets are connected. Then, the multi-band and multi-epoch VLBI of physics observations are analyzed. In the process of the jet component motion, there are the linear proper motion properties of Gaussian model-fitting of projection trajectory jet motion parameters, which can be used to explain each component of 0528 + 134 of the apparent superluminal phenomenon and flow density changes over time. The physics object is well computation.
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