Constraints on black hole accretion in V Puppis
Constraints on black hole accretion in V Puppis
 
  In light of the recent suggestion that the nearby eclipsing binary star system V Puppis has a dark companion on a long orbit, we present the results of radio and X-ray observations of it. We find an upper limit on its radio flux of about 300 ?Jy and a detection of it in the X-rays with a luminosity of about 3 × 1031 erg s?1, a value much lower than what had been observed in some of the low angular resolution surveys of the past. These data are in good agreement with the idea that the X-ray emission from V Puppis comes from mass transfer between the two B stars in the system, but can still accommodate the idea that the X-ray emission comes from the black hole accreting stellar wind from one or both of the B stars
  stars, individual, V Puppis, X-rays
  
  
  1070
  
    
      Maccarone, Thomas J.
      
        27e6101c-8fa4-41db-ba75-d2ee3d1a0c53
      
     
  
    
      Fender, Robert P.
      
        c802ddfc-25a3-4c0e-899d-11c405c705d1
      
     
  
    
      Knigge, Christian
      
        ac320eec-631a-426e-b2db-717c8bf7857e
      
     
  
    
      Tzioumis, A. K.
      
        d069871e-6e05-4f5a-a876-58fc583346c6
      
     
  
  
   
  
  
    
      2009
    
    
  
  
    
      Maccarone, Thomas J.
      
        27e6101c-8fa4-41db-ba75-d2ee3d1a0c53
      
     
  
    
      Fender, Robert P.
      
        c802ddfc-25a3-4c0e-899d-11c405c705d1
      
     
  
    
      Knigge, Christian
      
        ac320eec-631a-426e-b2db-717c8bf7857e
      
     
  
    
      Tzioumis, A. K.
      
        d069871e-6e05-4f5a-a876-58fc583346c6
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Maccarone, Thomas J., Fender, Robert P., Knigge, Christian and Tzioumis, A. K.
  
  
  
  
   
    (2009)
  
  
    
    Constraints on black hole accretion in V Puppis.
  
  
  
  
    Monthly Notices of the Royal Astronomical Society, 393 (3), .
  
   (doi:10.1111/j.1365-2966.2008.14291.x). 
  
  
   
  
  
  
  
  
   
  
    
      
        
          Abstract
          In light of the recent suggestion that the nearby eclipsing binary star system V Puppis has a dark companion on a long orbit, we present the results of radio and X-ray observations of it. We find an upper limit on its radio flux of about 300 ?Jy and a detection of it in the X-rays with a luminosity of about 3 × 1031 erg s?1, a value much lower than what had been observed in some of the low angular resolution surveys of the past. These data are in good agreement with the idea that the X-ray emission from V Puppis comes from mass transfer between the two B stars in the system, but can still accommodate the idea that the X-ray emission comes from the black hole accreting stellar wind from one or both of the B stars
        
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      Published date: 2009
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
     
        Keywords:
        stars, individual, V Puppis, X-rays
      
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 144181
        URI: http://eprints.soton.ac.uk/id/eprint/144181
        
          
        
        
        
          ISSN: 1365-2966
        
        
          PURE UUID: c1962ecf-30f8-4914-8414-7aa369cd3b4f
        
  
    
        
          
        
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
  
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  Date deposited: 16 Apr 2010 15:59
  Last modified: 09 Apr 2025 17:50
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      Contributors
      
          
          Author:
          
            
            
              Thomas J. Maccarone
            
          
        
      
          
          Author:
          
            
            
              Robert P. Fender
            
          
        
      
        
      
          
          Author:
          
            
            
              A. K. Tzioumis
            
          
        
      
      
      
    
  
   
  
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