arXiv · astro-ph/9809248
Relation between millimeter wavelengths emission and high-energy emission for active galactic nuclei
Abstract
After comparing the flux densities of a sample of active galactic nuclei detected by energetic gamma-ray experiment telescope at 90 and 230 GHz with the $γ$-ray emissions detected by Compton Gamma Ray Observatory and x-ray emission, a strong correlation between the emissions at the millimeter wavelength and the $γ$-ray emission is found. The average flux density of x-ray is almost proportional to the average flux density at the millimeter wavelength for quasars detected by energetic gamma-ray experiment telescope, which strongly supports the previous idea that the x-ray emissions of this kind sources are mainly produced by Synchrotron Self-Compton process.
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L. H. Huang, D. R. Jiang, Xinwu Cao. 1998-09-21. Relation between millimeter wavelengths emission and high-energy emission for active galactic nuclei. https://doi.org/10.1088/0256-307x%2F15%2F11%2F027
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