Hollow Core ?

نویسندگان

  • G. J. Qiao
  • J. F. Liu
  • Yang Wang
  • X. J. Wu
  • J. L. Han
چکیده

We carried out the Gaussian fitting to the profile of PSR B1237+25 and found that six components rather than five are necessary to make a good fit. In the central part, we found that the core emission is not filled pencil beam but is a small hollow cone. This implies that the impact angle could be β < 0.5 •. The " hollow core " is in agreement with Inverse Compton Scattering model of radio pulsars.

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تاریخ انتشار 1999