|                                   
                                        
  EGRET活动星系核的VLBI观测研究 
  洪晓瑜 蒋栋荣 王伟华 安 涛 
  (中国科学院上海天文台 上海 200030) 
  (中国科学院国家天文台 北京 100012) 
  摘    要                                
                                   
                                  
   
                                     
                        
                          
          |                       
                 
            EGRET空间望远镜已检测到66颗高置信度的g 
            射线活动星系核。这些活动星系核都是射电强的,具有很高的光度,迅速的光学变化,有相当的比例是视超光速源。对g 
            射线活动星系核的研究是目前世界上最活跃的前沿课题之一。为了完备EGRET 
            活动星系核的射电观测图像样本,以便进行更可信的统计研究。对一些缺少射电图像观测的EGRET活动星系核进行了多历元的VLBI和VLA的观测研究,得到了它们的射电结构图像。                     
            |                      
                          
                          
          |                       
                                  
                                     
           |                   
                       
                     
      | 关键词 |                 
      活动星系核 - 
        射电喷流 - 
        g 
        射线 - 
        VLBI |                    
                        
                       
      | 分类号 |                    
      P157.6 |                    
                        
                        
                         
                                  
                                  
                                  
  VLBI Observations of EGRET-detected AGNs                               
  Hong 
  Xiaoyu   Jiang Dongrong   
  Wang Weihua   An Tao 
  (Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 
  200030) 
  (Chinese Astronomical Observatories, Chinese Academy of Sciences, Beijing 
  100012) 
                                  
  Abstract                           
                  
                    
                    
                      
        |                 
               
          66 active galactic nuclei (AGNs) with high-confidence level have been 
          detected by EGRET identification. All these AGNs are the radio bright, 
          with the dramatic peak of the luminosity spectra at g-ray 
          frequencies, rapid optical variability, and the high fraction of 
          superluminal sources. To investigate the relation between the g-ray 
          emission and the radio structure, we observed a subsample of EGRET 
          sources with VLBI and VLA, which radio images are absent in the 
          literature. These results will be useful for the statistical research.  |                    
                          
                         
        |      |                    
                          
                         
        | Key words |                           
        AGNs 
          - 
          Jet - 
          Gamma-ray - VLBI |                    
                          
                         
         |                    
                          
                        
                       
                      
                                 
                               
                                
                               
  
                               
 |