标题： 活动星系核毫米波段发射与高能发射之间的关系 显示英文标题

标题： Relation between millimeter wavelengths emission and high-energy emission for active galactic nuclei

摘要： 通过对由高能伽马射线实验望远镜探测到的活动星系核样本在90 GHz和230 GHz的流量密度与由康普顿伽马射线天文台探测到的$\gamma$射线发射以及X射线发射进行比较，发现毫米波段发射与$\gamma$射线发射之间存在强相关性。对于由高能伽马射线实验望远镜探测到的类星体，X射线的平均流量密度几乎与毫米波长处的平均流量密度成正比，这强烈支持了先前的观点，即此类源的X射线发射主要由同步自康普顿过程产生。 显示英文摘要

摘要： 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 $\gamma$-ray emissions detected by Compton Gamma Ray Observatory and x-ray emission, a strong correlation between the emissions at the millimeter wavelength and the $\gamma$-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.