Correlation Between Radio-Millimeter and Gamma Ray Fluxes From Blazars

Details Correlation Between Radio-Millimeter and Gamma Ray Fluxes From Blazars Correlation Between Radio-Millimeter and Gamma Ray Fluxes From Blazars

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...19312206g&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #122.06; Bulletin of the American Astronomical Society, Vol. 31, p.665

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Using multifrequency databases, we have plotted radio (5 GHz, 22 GHz, and 37 GHz) and millimeter (90 GHz and 230 GHz) fluxes versus MeV and GeV g-ray fluxes of the EGRET blazar sample. Strong correlations have been found between the emissions at the radio-millimeter wavelengths and the gamma-rays. These correlations have been explained in the frame work of Synchrotron Self-Compton (SSC) processes between the radio-millimeter synchrotron emissions and the shock-accelerated electrons in the jets of blazars. Using this SSC model we are able to explain the GeV spectra of the EGRET blazars. The present model will also explain the physics of TeV flares in blazars and the time lag between the TeV and GeV photons from a blazar.

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