 
  
  
   
  Observed pop contains older slow pulsars
   Observed pop contains older slow pulsars 
 
  Old fast pulsars may have left the Galaxy
   Old fast pulsars may have left the Galaxy 
 
  Calibration of distances is vital
   Calibration of distances is vital 
 
  Must use sample of young pulsars
   Must use sample of young pulsars 
 
  
       km/s
  km/s 
 
  Can only results from Asymmetric SN
   Can only results from Asymmetric SN
 
  Potential implications for gamma ray bursts
   Potential implications for gamma ray bursts
 
  Very extended population of old pulsars
   Very extended population of old pulsars