The shape of pulsar emission patterns

Details The shape of pulsar emission patterns The shape of pulsar emission patterns

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..529g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, May-June 1991, p. 529-537. In Russian.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Pulsars, Stellar Models, Ellipticity, Radiation Sources, Radio Astronomy

Scientific paper

The dependence of the shape and width of the pulsar radiation pattern on the pulsar period is investigated on the basis of pulse profiles in the limited interval of wavelengths of about 260 pulsars. The relative pulse duration is compared with the ratio of numbers of pulsars to single and multicomponent pulses. It is shown that the simple circular-hollow-cone model does not agree with observational data. Preliminary estimates indicate that young pulsars (with short periods) have an elongated pattern which at long periods becomes circular. In the case of an elliptical pattern, the exact dependence of the observable width of the radiation beam on the basic angles is obtained.

Affiliated with

Also associated with

No associations

Rating

The shape of pulsar emission patterns 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 The shape of pulsar emission patterns, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The shape of pulsar emission patterns will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1279727