The radio/gamma-ray connection in AGNs
A. Lähteenmäki, M. Tornikoski
E. Valtaoja
Abstract
We have continued the comparison of the Metsähovi total flux density
radio variations, supplemented by very high frequency radio data, and EGRET
gamma-ray observations from Cycles 1-4. This work supplements the arguments
presented at the 4th Compton Symposium but also reports new results obtained
from the analysis of additional source properties.
We discuss the relationship between the two frequency regions and the
consequences it has on the source modeling. It seems that the radio emission
and the gamma-rays originate within the same shocked area of the relativistic
jet and that the gamma-rays are most likely produced by the synchrotron
self-Compton mechanism.
File translated from TEX by TTH, version 2.32.
On 16 Jul 1999, 09:18.