Pulsar average waveforms and hollow cone beam models

Details Pulsar average waveforms and hollow cone beam models Pulsar average waveforms and hollow cone beam models

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pawh.book.....b&link_type=abstract

NASA Tech. Memo., NASA-TM-X--70917; X--693-75-138, 44 p.

Astronomy and Astrophysics

Astronomy

28

Astronomical Models, Collimation, Pulsars, Waveforms, Extraterrestrial Radio Waves, Histograms, Radio Astronomy, Radio Frequencies, Radio Spectra

Scientific paper

An analysis of pulsar average waveforms at radio frequencies from 40 MHz to 15 GHz is presented. The analysis is based on the hypothesis that the observer sees one cut of a hollow-cone beam pattern and that stationary properties of the emission vary over the cone. The distributions of apparent cone widths for different observed forms of the average pulse profiles (single, double/unresolved, double/resolved, triple and multiple) are in modest agreement with a model of a circular hollow-cone beam with random observer-spin axis orientation, a random cone axis-spin axis alignment, and a small range of physical hollow-cone parameters for all objects.

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