X-ray Emission From Hot Polar Cap In Pulsars With Drifting Subpulses

Details X-ray Emission From Hot Polar Cap In Pulsars With Drifting Subpulses X-ray Emission From Hot Polar Cap In Pulsars With Drifting Subpulses

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...2e..30g&link_type=abstract

On the Present and Future of Pulsar Astronomy, 26th meeting of the IAU, Joint Discussion 2, 16-17 August, 2006, Prague, Czech Re

Astronomy and Astrophysics

Astronomy

Scientific paper

Within the framework of the partially screened inner acceleration region the relationship between the X-ray luminosity and the circulational periodicity of drifting sub-pulses is derived. This relationship is quite well satisfied in pulsars for which an appropriate radio and X-ray measurements exist. A special case of PSR B0943+10 is presented and discussed. The problem of formation of a partially screened inner acceleration region for all pulsars with drifting sub-pulses is also considered. It is argued that an efficient inner acceleration region just above the polar cap can be formed in a very strong and curved non-dipolar surface magnetic field.

Affiliated with

Also associated with

No associations

Rating

X-ray Emission From Hot Polar Cap In Pulsars With Drifting Subpulses does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with X-ray Emission From Hot Polar Cap In Pulsars With Drifting Subpulses, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray Emission From Hot Polar Cap In Pulsars With Drifting Subpulses will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1781790