Millimeter-wave behavior of EGRET-detected and non-EGRET-detected AGNs

Details Millimeter-wave behavior of EGRET-detected and non-EGRET-detected AGNs Millimeter-wave behavior of EGRET-detected and non-EGRET-detected AGNs

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..510..377t&link_type=abstract

THE FIFTH COMPTON SYMPOSIUM. AIP Conference Proceedings, Volume 510, pp. 377-381 (2000).

Computer Science

4

Active And Peculiar Galaxies And Related Systems, Gamma-Ray

Scientific paper

We present results from an analysis of the radio properties of two samples of sources: 1. EGRET-detected AGNs and 2. relatively bright and densely sampled southern AGNs not detected with EGRET. The radio properties of the detected and non-detected sources show similarity. When analysing the millimeter flux curves it turns out that most of the EGRET-detections were made when the source was going through the initial stages of a radio flare. These results suggest that many sources that exhibit blazar-like behavior in the millimeter domain could be detected at gamma energies if observed during the initial growth stages of a strong radio flare. .

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