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Finding Young Pulsars next up previous
Next: Braking Indices and Evolution Up: Young Energetic pulsars Previous: Basic Properties

Finding Young Pulsars

 

tex2html_wrap_inline3922   tex2html_wrap_inline4700
tex2html_wrap_inline3922   Scattering tex2html_wrap_inline4704
tex2html_wrap_inline3922   Dispersion tex2html_wrap_inline4708
tex2html_wrap_inline3922  
tex2html_wrap_inline3922   Pulsar Spectral Index tex2html_wrap_inline4716
tex2html_wrap_inline3922   Young pulsars deep in Galactic plane
tex2html_wrap_inline3922   Implies high frequency surveys tex2html_wrap_inline4722 MHz

  
Figure 21: An example of a 1400 MHz survey. Filled circles are new pulsars, Open circles are previously known pulsars. From Johnston et al 1992 [16]


Jon Bell
Thu Dec 19 15:15:11 GMT 1996