Pulse Profile Simulations for PSR 1237+25 and PSR 1933+16

Details Pulse Profile Simulations for PSR 1237+25 and PSR 1933+16 Pulse Profile Simulations for PSR 1237+25 and PSR 1933+16

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cha%26a..23..133l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 23, Issue 2, p. 133-138.

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Empirical theory of pulsar radio emission emphasized that the emission beam consists of a central core and two concentric cones and pointed out that there exists two distinct trends in mean pulse profile evolution: the profile width increases in one and decreases in the other, as the observing frequency increases. Such a scenario rules out the hollow-cone beam model. In this paper, within the framework of the inverse Compton scattering model of pulsar radio emission, we present our simulations for PSR 1237+25 and PSR 1933+16, representatives of the two trends. The agreement of our results with the observations confirms the role inverse Compton scattering plays in the pulsar radio emission processes.

Affiliated with

Also associated with

No associations

Rating

Pulse Profile Simulations for PSR 1237+25 and PSR 1933+16 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 Pulse Profile Simulations for PSR 1237+25 and PSR 1933+16, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulse Profile Simulations for PSR 1237+25 and PSR 1933+16 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1029359