|                                       
                                            
  乌鲁木齐25m射电望远镜脉冲星观测研究     
  吴鑫基    
  1,2,3    
  张     
  晋 1,4      
  王     
  娜 1,2,3,4    艾  
  力.依 1,2,3,4      
  艾力.玉  
  1,4    
  (1.中国科学院乌鲁木齐天文站 乌鲁木齐 830011)  
  (2.北京大学天文学系 北京 100871)  
  (3.中国科学院北京大学联合北京天体物理中心 北京 100871)   
  (4.中国科学院国家天文台 北京 100012)  
  摘    要                                     
                                        
                                       
        
                                          
                             
                               
          |                            
                  
            乌鲁木齐天文站自1999年以来陆续研制完成脉冲星1.5GHz频段消色散接收系统,0.327GHz,0.61GHz,2.3GHz, 4.8GHz和8.4GHz等5个频段上的单通道的脉冲星接收系统和2组双频(2.3GHz和8.4GHz及0.327GHz和0.61GHz)同时观测的接收系统。上述设备均已投入观测,并取得一批诸如脉冲星周期参数、周期跃变、自行速度、脉冲轮廓模式变化、星际闪烁和谱特性等观测成果。                        
            |                         
                             
                             
          |                          
                                     
                                        
           |                      
                          
                        
      | 关键词 |                    
      脉冲星 -  
        观测 |                        
                            
                           
      | 分类号 |                        
      P145.6 |                        
                            
                            
                             
                                      
                                    
                                    
  The  
  Progress of Pulsar Observation at UAO                                   
  Wu Xinji 1,2,3  
    Zhang Jin 1,4    
  Wang Na 1,2,3,4    
  Esamdin Aili 1,2,3,4   
  Yusupu  
  Aili 1,4 
  
  (1.Urumqi Astronomical Observatory,Chinese Academy of  
  Sciences, Urumqi  830011)  
  (2.Department of Astronomy, Peking University, Beijing   
  100871)  
  (3. The Chinese Academy of Sciences-Peking University Joint Beijing  
  Astrophysics Center, Beijing  100871)  
  (4. National Astronomical Observatories, Chinese Academy of Sciences, Beijing   
  100012)  
  Abstract     
                      
                        
                        
                          
        |                     
               
          The 1.5GHz de-dispersion pulsar-timing observation system of UAO has 
          been made since 1999. We also built the single-channel receivers at 
          0.327GHz, 0.61GHz, 2.3GHz, 4.8GHz and 8.4GHz. And then the 
          simultaneous de-dispersion observation system at 2.3GHz and 8.4GHz and 
          the simultaneous single-channel  observation 
          system at 0.327GHz and 0.61GHz were successfully developed. Some 
          scientific results such as glitch, model changing, inter-stellar 
          scintillation and the spectra of pulsar, have been obtained by using 
          these equipments.  |                        
                              
                             
        |      |                        
                              
                             
        | Key words |                              
        pulsars 
          - 
          observation |                        
                              
                             
         |                        
                              
                            
                           
                          
                                     
                                   
                                    
                                   
  
                                   
 |