这些讨论表明，活动星系核的短时标光变特征对厚吸积盘模型提供了强有力的支持。
The conclusion is: the short term variability behavior provides a strong support to the thick accretion disk model of AGN.
并对两派观点争论的焦点问题进行了详细的阐述。这个焦点问题与活动星系核的X射线辐射紧密相关。
We discuss in detail on the focus between the arguments of the above two basic views which are very closely related to the X-ray radiation of active galactic nuclei.
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