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We discuss a model of formation of extragalactic radio sources when theparent optical galaxy has a large-scale dipolar magnetic field. The study ofdynamics of ejected from the central part of optical galaxy clouds ofrelativistic particles in dipolar magnetic field gives a possibility to explainmain morphological features and physical properties of formed extragalacticradio sources. We bring some results of statistical analyses and correlationsbetween physical parameters for more than 500 radio sources. In appendix wepresent the data of all used extragalactic radio sources with the referencesfor them.

The role of large-scale magnetic field in the morphology and evolution of extragalactic radio sources