Affiliation:
1. NAS RA V. Ambartsumian Byurakan Astrophysical Observatory (BAO), Armenia
Abstract
We discuss a model of formation of extragalactic radio sources when the parent optical galaxy has a large-scale dipolar magnetic field. The study of dynamics of ejected from the central part of optical galaxy clouds of relativistic particles in dipolar magnetic field gives a possibility to explain main morphological features and physical properties of formed extragalactic radio sources. We bring some results of statistical analyses and correlations between physical parameters for a large sample of extragalactic radio sources.
Publisher
NAS RA Byurakan Astrophysical Observatory after V. A. Ambartsumian
Subject
General Medicine,General Chemistry
Reference28 articles.
1. Ambartsumian, V. 1966, Transactions of the International Astronomical Union, Series B, 12, 578
2. Andreasyan, R. R., Hovhannisyan, M. A., Paronyan, G. M., & Abrahamyan, H. V. 2013, Astrophysics, 56, 382
3. Andreasyan, R. R. 2012, arXiv:1203.6549
4. Andreasyan, R. R., Martin, J.-M., & Paronyan, G. M. 2008, Astrophysics, 51, 454
5. Andreasyan, R. R., Appl, S., & Sol, H. 2002, Astrophysics, 45, 198
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