Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.atnf.csiro.au/research/pulsar/Tutorial/tut/node48.html
Дата изменения: Unknown
Дата индексирования: Tue Feb 5 00:38:12 2013
Кодировка:
Поисковые слова: wmap

Basic Properties

 

  t < 100,000 years
  Short periods ms
  Large period derivatives
  Strong magnetic fields Gauss
  Close to Galactic plane

  
Table 1: Young Energetic Radio Pulsars. O - optical, X - X-rays, - -rays, I - infra-red, U - ultraviolet, J - jet, N - nebula, G - glicthes, BU - bullets, B - bow shock, Y - yes, P - probably, N - no, ? - maybe

  Vast array of phenomena result from large

  
Figure 20: The radio pulsar equivalent of the Hertzsprung-Russell diagram - a physical diagram indicating the nature and evolution of neutron stars. Each dot represents a pulsar, stars represent pulsars associated with supernova remnants, circles indicate pulsars in binary systems and ellipses indicate pulsars in binary systems with eccentric orbits.