Pulsar beams - conal not patchy

Details Pulsar beams - conal not patchy Pulsar beams - conal not patchy

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.280..143g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 280, Issue 1, pp. 143-148.

Astronomy and Astrophysics

Astronomy

21

Pulsars: General, Pulsars: Individual: Psr 1133+16, Pulsars: Individual: Psr 0320+39, Pulsars: Individual: Psr 2016+28

Scientific paper

We analyse the frequency dependence of pulsar characteristics and conclude that, within the angular beaming model of pulsar radiation modulation, the longitudes of subpulses should be weakly dependent on frequency as compared with the longitudes of profile components. This is actually observed in pulsars. Based on this conclusion, we argue that the structure of mean pulsar beams is conal and not patchy.

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