Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients
Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients
 
  We report on a first census of Galactic black hole X-ray binary (BHXRB)
properties with the second data release (DR2) of Gaia, focusing on
dynamically confirmed and strong candidate BH transients. Gaia DR2
provides five-parameter astrometric solutions including position,
parallax and proper motion for 11 out of a sample of 24 systems.
Distance estimates are tested with parallax inversion as well as
Bayesian inference. We derive an empirically motivated characteristic
scalelength of L = 2.17 ± 0.12 kpc for this BHXRB population to
infer distances based upon an exponentially decreasing space density
prior. Geometric DR2 parallaxes provide new, independent distance
estimates, but the faintness of this population in quiescence results in
relatively large fractional distance uncertainties. Despite this, DR2
estimates generally agree with the distances found in the literature.
The most discrepant case is BW Cir, for which detailed studies of the
donor star have suggested a distant location at ≳25 kpc. The large
parallax and relatively high proper motion measured by DR2 instead
indicate significantly smaller distances, suggesting that the source
might be amongst the nearest of XRBs. However, both larger and smaller
distances create problems for the interpretation of the source, and
follow-up data are required to resolve its true nature. DR2 also
provides a first distance estimate to one source, MAXI J1820+070, and
novel proper motion estimates for seven sources. Peculiar velocities
relative to Galactic rotation exceed ≈ 50 km s-1 for the
bulk of the sample, with a median system kinetic energy of peculiar
motion of ˜ 5 × 1047 erg. BW Cir could be a new
high-velocity BHXRB if its astrometry is confirmed. A putative
anticorrelation between peculiar velocity and BH mass is found, as
expected in mass-dependent BH kick formation channels, but this trend
remains weak in the DR2 data.
  accretion, accretion discs, parallaxes, proper motions, stars: black holes, stars: distances
  
  
  2642-2655
  
    
      Gandhi, Poshak
      
        5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
      
     
  
    
      Rao, Anjali
      
        3a3aa402-cf58-4724-9e63-fe9fdc6f39a6
      
     
  
    
      Johnson, Michael A. C.
      
        33a0d8cb-491b-4b3f-b193-540a331ac705
      
     
  
    
      Paice, John A.
      
        0ccafe5a-82d8-40bf-8b73-f71a841ac550
      
     
  
    
      Maccarone, Thomas J.
      
        c2f1d87b-e2ef-4e33-b09f-a2861d917ea8
      
     
  
  
   
  
  
    
    
  
    
    
  
    
      May 2019
    
    
  
  
    
      Gandhi, Poshak
      
        5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
      
     
  
    
      Rao, Anjali
      
        3a3aa402-cf58-4724-9e63-fe9fdc6f39a6
      
     
  
    
      Johnson, Michael A. C.
      
        33a0d8cb-491b-4b3f-b193-540a331ac705
      
     
  
    
      Paice, John A.
      
        0ccafe5a-82d8-40bf-8b73-f71a841ac550
      
     
  
    
      Maccarone, Thomas J.
      
        c2f1d87b-e2ef-4e33-b09f-a2861d917ea8
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Gandhi, Poshak, Rao, Anjali, Johnson, Michael A. C., Paice, John A. and Maccarone, Thomas J.
  
  
  
  
   
    (2019)
  
  
    
    Gaia Data Release 2 distances and peculiar velocities for Galactic black hole transients.
  
  
  
  
    Monthly Notices of the Royal Astronomical Society, 485 (2), .
  
   (doi:10.1093/mnras/stz438). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          We report on a first census of Galactic black hole X-ray binary (BHXRB)
properties with the second data release (DR2) of Gaia, focusing on
dynamically confirmed and strong candidate BH transients. Gaia DR2
provides five-parameter astrometric solutions including position,
parallax and proper motion for 11 out of a sample of 24 systems.
Distance estimates are tested with parallax inversion as well as
Bayesian inference. We derive an empirically motivated characteristic
scalelength of L = 2.17 ± 0.12 kpc for this BHXRB population to
infer distances based upon an exponentially decreasing space density
prior. Geometric DR2 parallaxes provide new, independent distance
estimates, but the faintness of this population in quiescence results in
relatively large fractional distance uncertainties. Despite this, DR2
estimates generally agree with the distances found in the literature.
The most discrepant case is BW Cir, for which detailed studies of the
donor star have suggested a distant location at ≳25 kpc. The large
parallax and relatively high proper motion measured by DR2 instead
indicate significantly smaller distances, suggesting that the source
might be amongst the nearest of XRBs. However, both larger and smaller
distances create problems for the interpretation of the source, and
follow-up data are required to resolve its true nature. DR2 also
provides a first distance estimate to one source, MAXI J1820+070, and
novel proper motion estimates for seven sources. Peculiar velocities
relative to Galactic rotation exceed ≈ 50 km s-1 for the
bulk of the sample, with a median system kinetic energy of peculiar
motion of ˜ 5 × 1047 erg. BW Cir could be a new
high-velocity BHXRB if its astrometry is confirmed. A putative
anticorrelation between peculiar velocity and BH mass is found, as
expected in mass-dependent BH kick formation channels, but this trend
remains weak in the DR2 data.
         
      
      
        
          
            
  
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     - Accepted Manuscript
   
  
  
    
  
 
          
            
          
            
           
            
           
        
        
       
    
   
  
  
  More information
  
    
      Accepted/In Press date: 4 February 2019
 
    
      e-pub ahead of print date: 14 March 2019
 
    
      Published date: May 2019
 
    
  
  
    
  
    
  
    
  
    
  
    
     
    
  
    
     
        Keywords:
        accretion, accretion discs, parallaxes, proper motions, stars: black holes, stars: distances
      
    
  
    
  
    
  
  
        Identifiers
        Local EPrints ID: 430017
        URI: http://eprints.soton.ac.uk/id/eprint/430017
        
          
        
        
        
          ISSN: 1365-2966
        
        
          PURE UUID: 2054fb94-354d-4799-a814-8b2b23ddbf6c
        
  
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
        
          
        
    
  
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  Date deposited: 10 Apr 2019 16:30
  Last modified: 10 Apr 2025 01:52
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      Contributors
      
        
      
          
          Author:
          
            
            
              Anjali Rao
            
          
        
      
          
          Author:
          
            
              
              
                Michael A. C. Johnson
              
              
                 
              
            
            
          
         
      
          
          Author:
          
            
            
              John A. Paice
            
          
        
      
          
          Author:
          
            
            
              Thomas J. Maccarone
            
          
        
      
      
      
    
  
   
  
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