Kumar, P;
              
      
            
                McMahon, E;
              
      
            
                Panaitescu, A;
              
      
            
                Willingale, R;
              
      
            
                O'Brien, P;
              
      
            
                Burrows, D;
              
      
            
                Cummings, J;
              
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
          
      
            
            
            ... Zane, S; + view all
            
          
      
        
        
        
    
  
(2007)
  The nature of the outflow in gamma-ray bursts.
Monthly Notices of the Royal Astronomical Society: Letters
, 376
       (1)
    
     L57 - L61.
    
         10.1111/j.1365-2966.2007.00286.x.
  
  
      
    
  
Preview  | 
            
              
PDF
 174439.pdf Download (135kB)  | 
          
Abstract
The Swift satellite has enabled us to follow the evolution of gamma-ray burst (GRB) fireballs from the prompt gamma-ray emission to the afterglow phase. The early-time X-ray and optical data for GRBs obtained by telescopes aboard the Swift satellite show that the source for prompt gamma-ray emission, the emission that heralds these bursts, is short lived, and is distinct from the source for the long-lived afterglow emission that follows the initial burst. Using these data we determine the distance of the gamma-ray source from the centre of the explosion. We find this distance to be 10(15)-10(16) cm for most bursts, and show that this is within a factor of about 10 of the radius of the shock heated circumstellar medium (CSM) producing the X-ray photons. Furthermore, using the early gamma-ray, X-ray and optical data we show that the prompt gamma-ray emission cannot be produced in internal shocks nor can it be produced in the external shock; in a more general sense gamma-ray generation mechanisms based on shock physics have problems explaining the GRB data for ten Swift bursts analyzed in this work. A magnetic field dominated outflow model for GRBs has a number of attractive features, although evidence in its favour is inconclusive. Finally, the X-ray and optical data allow us to provide an upper limit on the density of the CSM of about 10 protons cm(-3) at a distance of similar to 5 x 10(16) cm from the centre of explosion.
| Type: | Article | 
|---|---|
| Title: | The nature of the outflow in gamma-ray bursts | 
| Open access status: | An open access version is available from UCL Discovery | 
| DOI: | 10.1111/j.1365-2966.2007.00286.x | 
| Publisher version: | http://dx.doi.org/10.1111/j.1365-2966.2007.00286.x | 
| Language: | English | 
| Additional information: | © 2007 RAS Definitive versions of articles pre-2013 are available at http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966, now published by http://mnras.oxfordjournals.org | 
| Keywords: | gamma-rays : bursts, gamma-rays : theory, AFTERGLOW EMISSION, MAGNETIC-FIELDS, LIGHT-CURVE, FIREBALLS, PULSARS, PROMPT, MODEL | 
| UCL classification: | UCL UCL > Provost and Vice Provost Offices UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics  | 
        
| URI: | https://discovery.ucl.ac.uk/id/eprint/174439 | 
Archive Staff Only
![]()  | 
        View Item | 
                      
