Identifying a new intermediate SFXT: discovering a 30 day period in SAX J1818.6—1703
Identifying a new intermediate SFXT: discovering a 30 day period in SAX J1818.6—1703
 
  Supergiant fast X-ray transients (SFXTs) are recently discovered members of the expanding family of high mass X-ray binaries. They represent a population of sources which show transient activity and are associated with blue supergiant optical counterparts. To date INTEGRAL has observed 9 SFXTs; three of which have been conformed to be X-ray pulsars. The fast, transient nature of these sources makes them a challenge to study and understand. Recently, periodic behaviour has been discovered in three such systems and has been attributed to orbital motion. We present here the discovery of a 30 day period in SAX J1818.6-1703.
  
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      Hill, A.B.
      
        b1007941-b5b1-47cd-8476-7c6b9c57f347
      
     
  
    
      Bird, A.J.
      
        045ee141-4720-46fd-a412-5aa848a91b32
      
     
  
    
      Bazzano, A.
      
        8eef0c6e-1a5f-4bcd-a034-9a5c3b29104d
      
     
  
    
      McBride, V.A.
      
        a4608811-5a3f-4218-ada0-28f57ec2a0fd
      
     
  
    
      Sguera, V.
      
        371bb568-7e56-496e-a624-dba6de79d9e1
      
     
  
    
      Shaw, S.E.
      
        65776027-991a-45ae-8338-e1c73909ce64
      
     
  
    
      Watkins, H.J.
      
        fb25318a-fc6a-4b07-963a-d5c27a533a97
      
     
  
  
   
  
  
    
      11 May 2009
    
    
  
  
    
      Hill, A.B.
      
        b1007941-b5b1-47cd-8476-7c6b9c57f347
      
     
  
    
      Bird, A.J.
      
        045ee141-4720-46fd-a412-5aa848a91b32
      
     
  
    
      Bazzano, A.
      
        8eef0c6e-1a5f-4bcd-a034-9a5c3b29104d
      
     
  
    
      McBride, V.A.
      
        a4608811-5a3f-4218-ada0-28f57ec2a0fd
      
     
  
    
      Sguera, V.
      
        371bb568-7e56-496e-a624-dba6de79d9e1
      
     
  
    
      Shaw, S.E.
      
        65776027-991a-45ae-8338-e1c73909ce64
      
     
  
    
      Watkins, H.J.
      
        fb25318a-fc6a-4b07-963a-d5c27a533a97
      
     
  
       
    
 
  
    
      
  
  
  
  
    Hill, A.B., Bird, A.J., Bazzano, A., McBride, V.A., Sguera, V., Shaw, S.E. and Watkins, H.J.
  
  
  
  
   
    (2009)
  
  
    
    Identifying a new intermediate SFXT: discovering a 30 day period in SAX J1818.6—1703.
  
  
  
  
    
    
    
      
        
   
  
    Simbol-X: focusing on the hard x-ray universe: Proceedings of the 2nd International Simbol-X Symposium.
   
        
        
        
      
    
  
  
  
      
          
          
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   (doi:10.1063/1.3149444).
  
   
  
    
      Record type:
      Conference or Workshop Item
      (Paper)
      
      
    
   
    
      
        
          Abstract
          Supergiant fast X-ray transients (SFXTs) are recently discovered members of the expanding family of high mass X-ray binaries. They represent a population of sources which show transient activity and are associated with blue supergiant optical counterparts. To date INTEGRAL has observed 9 SFXTs; three of which have been conformed to be X-ray pulsars. The fast, transient nature of these sources makes them a challenge to study and understand. Recently, periodic behaviour has been discovered in three such systems and has been attributed to orbital motion. We present here the discovery of a 30 day period in SAX J1818.6-1703.
        
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      Published date: 11 May 2009
 
    
  
  
    
  
    
  
    
     
        Venue - Dates:
        Simbol-X: focusing on the hard x-ray universe: Proceedings of the 2nd International Simbol-X Symposium, 2009-05-11
      
    
  
    
  
    
     
    
  
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 144781
        URI: http://eprints.soton.ac.uk/id/eprint/144781
        
          
        
        
        
        
          PURE UUID: c46ffde1-236c-4949-bf8e-0a636e0db760
        
  
    
        
          
            
              
            
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
  
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  Date deposited: 25 May 2010 11:21
  Last modified: 14 Mar 2024 02:48
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      Contributors
      
          
          Author:
          
            
              
              
                A.B. Hill
              
              
                 
              
            
            
          
         
      
        
      
          
          Author:
          
            
            
              A. Bazzano
            
          
        
      
          
          Author:
          
            
            
              V.A. McBride
            
          
        
      
          
          Author:
          
            
            
              V. Sguera
            
          
        
      
          
          Author:
          
            
            
              S.E. Shaw
            
          
        
      
          
          Author:
          
            
            
              H.J. Watkins
            
          
        
      
      
      
    
  
   
  
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