The radio/gamma-ray connection in AGNs

Details The radio/gamma-ray connection in AGNs The radio/gamma-ray connection in AGNs

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..372l&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 372-376 (2000).

Astronomy and Astrophysics

Astronomy

5

Active And Peculiar Galaxies And Related Systems, Radiation Mechanisms, Polarization, Astronomical Observations

Scientific paper

We have continued the comparison of the Metsähovi total flux density radio variations and EGRET gamma-ray observations from Cycles 1-4. This work compliments the arguments presented at the 4th Compton Symposium. We have also attempted to remove the effect that different radio and gamma-ray spectral indices have on the observed 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 (SSC) mechanism. .

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