Detection of white dwarf companions to blue straggler stars from UVIT observations of M67
Detection of white dwarf companions to blue straggler stars from UVIT observations of M67
 
  We investigate the old open cluster M67 using ultraviolet photometric data of Ultra-Violet Imaging Telescope in multi-filter far-UV bands. M67, well known for the presence of several blue straggler stars (BSS), has been put to detailed tests to understand their formation pathways. Currently, there are three accepted formation channels: mass transfer due to Roche-lobe overflow in binary systems, stellar mergers either due to dynamical collisions or through coalescence of close binaries. So far, there had not been any confirmed detection of a white dwarf (WD) companion to any of the BSSs in this cluster. Here, we present the detection of WD companions to 5 bright BSSs in M67. The multiwavelength spectral energy distributions covering 0.12 -11.5 $\mu$m range, were found to require binary spectral fits for 5 BSSs, consisting of a cool (BSS) and a hot companion. The parameters (Luminosity, Temperature, Radius and Mass) of the hot companions suggest them to be WDs with mass in the range 0.2 - 0.35 M$_{\odot}$ with T$_{eff}$ $\sim$ 11000 - 24000 K.
  astro-ph.SR, astro-ph.GA
  
  1-4
  
    
      Sindhu, N
      
        317ad9d0-998f-416a-9033-c57572df15c4
      
     
  
    
      Subramaniam, Annapurni
      
        6a91cb92-e7e8-40cb-b457-cc5abac5e924
      
     
  
    
      Geller, Aaron M
      
        358fcd0f-def3-47e2-8595-ab16cdb12f3a
      
     
  
    
      Jadhav, Vikrant
      
        7a9cc29e-74ab-4d79-8c16-3ac2b057feb1
      
     
  
    
      Knigge, Christian
      
        ac320eec-631a-426e-b2db-717c8bf7857e
      
     
  
    
      Simunovic, Mirko
      
        ce9a236f-751d-49c4-90e9-b53fa8a6a028
      
     
  
    
      Leigh, Nathan
      
        90069e68-a317-4cce-92e3-2401e3518751
      
     
  
    
      Shara, Michael
      
        bac39df6-4548-4335-a751-9be1122e8c33
      
     
  
    
      Puzia, Thomas H
      
        b625d688-ed67-462d-9691-6e7f9b69807b
      
     
  
  
   
  
  
    
      5 August 2019
    
    
  
  
    
      Sindhu, N
      
        317ad9d0-998f-416a-9033-c57572df15c4
      
     
  
    
      Subramaniam, Annapurni
      
        6a91cb92-e7e8-40cb-b457-cc5abac5e924
      
     
  
    
      Geller, Aaron M
      
        358fcd0f-def3-47e2-8595-ab16cdb12f3a
      
     
  
    
      Jadhav, Vikrant
      
        7a9cc29e-74ab-4d79-8c16-3ac2b057feb1
      
     
  
    
      Knigge, Christian
      
        ac320eec-631a-426e-b2db-717c8bf7857e
      
     
  
    
      Simunovic, Mirko
      
        ce9a236f-751d-49c4-90e9-b53fa8a6a028
      
     
  
    
      Leigh, Nathan
      
        90069e68-a317-4cce-92e3-2401e3518751
      
     
  
    
      Shara, Michael
      
        bac39df6-4548-4335-a751-9be1122e8c33
      
     
  
    
      Puzia, Thomas H
      
        b625d688-ed67-462d-9691-6e7f9b69807b
      
     
  
       
    
 
  
    
      
  
  
  
  
    Sindhu, N, Subramaniam, Annapurni, Geller, Aaron M, Jadhav, Vikrant, Knigge, Christian, Simunovic, Mirko, Leigh, Nathan, Shara, Michael and Puzia, Thomas H
  
  
  
  
   
    (2019)
  
  
    
    Detection of white dwarf companions to blue straggler stars from UVIT observations of M67.
  In, 
  
    
  
  
   
  IAU Symposium No. 351 proceedings - Star Clusters: From the Milky Way to the Early Universe, 2019. 
  
  
  
    (IAU Conference Series, 351)
  
  
    
       Star Clusters: from the Milky Way to the Early Universe (27/05/19 - 31/05/19)
    
  
  
  
  
  
      
  .
  
  
  
  (doi:10.1017/S1743921319006975).
  
   
  
    
      Record type:
      Book Section
      
      
      
    
   
    
    
      
        
          Abstract
          We investigate the old open cluster M67 using ultraviolet photometric data of Ultra-Violet Imaging Telescope in multi-filter far-UV bands. M67, well known for the presence of several blue straggler stars (BSS), has been put to detailed tests to understand their formation pathways. Currently, there are three accepted formation channels: mass transfer due to Roche-lobe overflow in binary systems, stellar mergers either due to dynamical collisions or through coalescence of close binaries. So far, there had not been any confirmed detection of a white dwarf (WD) companion to any of the BSSs in this cluster. Here, we present the detection of WD companions to 5 bright BSSs in M67. The multiwavelength spectral energy distributions covering 0.12 -11.5 $\mu$m range, were found to require binary spectral fits for 5 BSSs, consisting of a cool (BSS) and a hot companion. The parameters (Luminosity, Temperature, Radius and Mass) of the hot companions suggest them to be WDs with mass in the range 0.2 - 0.35 M$_{\odot}$ with T$_{eff}$ $\sim$ 11000 - 24000 K.
         
      
      
        
          
            
  
    Text
 1908.01573v1
     - Accepted Manuscript
   
  
  
    
  
 
          
            
          
            
           
            
           
        
        
       
    
   
  
  
  More information
  
    
      Published date: 5 August 2019
 
    
  
  
    
  
    
     
        Additional Information:
        4 pages, 2 figures, to appear in IAU Symposium No. 351 proceedings - Star Clusters: From the Milky Way to the Early Universe, 2019
      
    
  
    
     
        Venue - Dates:
        Star Clusters: from the Milky Way to the Early Universe, , Bologna, Italy, 2019-05-27 - 2019-05-31
      
    
  
    
  
    
  
    
     
        Keywords:
        astro-ph.SR, astro-ph.GA
      
    
  
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 433869
        URI: http://eprints.soton.ac.uk/id/eprint/433869
        
          
        
        
        
        
          PURE UUID: 84220666-0367-4ba7-8ff2-969a39bc76e7
        
  
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
            
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
        
          
        
    
  
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  Date deposited: 05 Sep 2019 16:30
  Last modified: 16 Mar 2024 03:58
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      Contributors
      
          
          Author:
          
            
            
              N Sindhu
            
          
        
      
          
          Author:
          
            
            
              Annapurni Subramaniam
            
          
        
      
          
          Author:
          
            
            
              Aaron M Geller
            
          
        
      
          
          Author:
          
            
            
              Vikrant Jadhav
            
          
        
      
        
      
          
          Author:
          
            
            
              Mirko Simunovic
            
          
        
      
          
          Author:
          
            
            
              Nathan Leigh
            
          
        
      
          
          Author:
          
            
            
              Michael Shara
            
          
        
      
          
          Author:
          
            
            
              Thomas H Puzia
            
          
        
      
      
      
    
  
   
  
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