Thermal X-ray emission from hot polar cap in drifting subpulse pulsars

Details Thermal X-ray emission from hot polar cap in drifting subpulse pulsars Thermal X-ray emission from hot polar cap in drifting subpulse pulsars

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.308..325g&link_type=abstract

Astrophysics and Space Science, Volume 308, Issue 1-4, pp. 325-333

Astronomy and Astrophysics

Astrophysics

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 subpulses 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 subpulses 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

Thermal X-ray emission from hot polar cap in drifting subpulse pulsars 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 Thermal X-ray emission from hot polar cap in drifting subpulse pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Thermal X-ray emission from hot polar cap in drifting subpulse pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1682399