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Relation Between Millimeter Wavelengths Emission and High-Energy Emission for Active Galactic Nuclei |
| HUANG Li-hua;JIANG Dong-rong;CAO Xin-wu |
| Shanghai Observatory, Chinese Academy of Sciences, Shanghai 200030 |
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| Cite this article: |
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HUANG Li-hua, JIANG Dong-rong, CAO Xin-wu 1998 Chin. Phys. Lett. 15 856-858 |
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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 emission 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 wave-length 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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98.54.Aj
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Published: 01 November 1998
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