Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-30T02:49:21.086Z Has data issue: false hasContentIssue false
  • English
  • Français

The Study of Extended Radio Galaxies

Published online by Cambridge University Press:  25 May 2016

M.A. Hovhannisyan
M.A. Hovhannisyan*
Affiliation:
Byurakan Astrophysical Observatory, Byurakan, 378433, Armenia

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The jets of radio galaxies have an essential role in the formation of their extended components. However, in general, the physical characteristics of the jets differ from the characteristics of the extended components (the spectra, polarisation, density and so on).

Type
II. Observational Properties of AGN and Related Objects
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 171
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Artyukh, V. S., & Hovhannisyan, M. A. 1988, Pisma AZh, 14, 706 Google Scholar
Artyukh, V. S., & Hovhannisyan, M. A. 1993, AZh, 70, 443 Google Scholar
Artyukh, V. S., Hovhannisyan, M. A., & Tyul'bashev, S. A. 1994, Pisma AZh, 20, 178 Google Scholar
Artyukh, V. S., Hovhannisyan, M. A., & Tyul'bashev, S. A. 1994, Pisma AZh, 20, 258 Google Scholar
Hovhannisyan, M. A. 1995, Astrofizika, 38, 692 Google Scholar