Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-06-20T07:22:12.956Z Has data issue: false hasContentIssue false
  • English
  • Français

Strong Radio Outbursts in Six Active Galactic Nuclei in 1997-1998

Published online by Cambridge University Press:  25 May 2016

Y.Y. Kovalev
Y.Y. Kovalev*
Affiliation:
Astro Space Center of the Lebedev Physical Institute, Profsoyuznaya 84/32, Moscow, 117810 Russia

Abstract

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 beginnings of strong radio flares in six AGNs were detected and their evolution was studied using 1–22 GHz five epoch instantaneous spectral observations in 1997–1998. The phenomena started at the highest frequency and moved to the lower frequency in a regular fashion. Such behavior of the flares in AGNs can be explained by synchrotron emission from a compact relativistic jet implying different physical models which are discussed. For different types of AGNs the same behavior of flares is revealed, in favor of the same basic physical model for BL Lacs and quasars. A birth of new VLBI components in compact jets associated with these outbursts is predicted.

Type
IV. AGN Related Phenomena
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 418 - 419
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Gabuzda, D.C., et al. 1994, ApJ, 435, 140 Google Scholar
Kovalev, Yu.A., & Mikhailutsa, V.P. 1980, Soviet Ast., 24, 400 Google Scholar
Kovalev, Yu.A. 1998, Bull. SAO, 44, 50 Google Scholar
Kovalev, Y.Y., & Larionov, G.M. 1994, ALett., 20, 3 Google Scholar
Marsher, A.P., & Gear, W.K. 1985, ApJ, 298, 114 Google Scholar