Relationships between radio and gamma-ray properties in active galactic nuclei

Details Relationships between radio and gamma-ray properties in active galactic nuclei Relationships between radio and gamma-ray properties in active galactic nuclei

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1452l&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1452-1456 (1997).

Computer Science

5

Active And Peculiar Galaxies And Related Systems, Gamma-Ray, Radio, Microwave, Quasars, Magnitudes And Colors, Luminosities

Scientific paper

We compare the Metsähovi 22 and 37 GHz total flux density variations of active galactic nuclei with EGRET Phase 1+2+3 gamma-ray data. There is a connection between the type of the source, the phase of the radio flare, the associated radio variability brightness temperature and the gamma-ray emission. It seems that the gamma emission originates within the same shocks which produce the synchrotron flares in radio-induced by the synchrotron self-Compton mechanism.

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