Pulsar average wave forms and hollow-cone beam models

Details Pulsar average wave forms and hollow-cone beam models Pulsar average wave forms and hollow-cone beam models

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...209..895b&link_type=abstract

Astrophysical Journal, vol. 209, Nov. 1, 1976, pt. 1, p. 895-907. Research supported by the National Radio Astronomy Observator

Astronomy and Astrophysics

Astronomy

103

Beams (Radiation), Pulsars, Stellar Models, Waveforms, Astronomical Catalogs, Error Analysis, Frequency Response, Histograms, Pencil Beams, Radio Frequencies, Supernovae

Scientific paper

Pulsar wave forms have been analyzed from observations conducted over a wide radio-frequency range to assess the wave-form morphologies and to measure wave-form widths. The results of the analysis compare favorably with the predictions of a model with a hollow-cone beam of fixed dimensions and with random orientation of both the observer and the cone axis with respect to the pulsar spin axis. A class of three-component wave forms is included in the model by adding a central pencil beam to the hollow-cone hypothesis. The consequences of a number of discrepancies between observations and quantitative predictions of the model are discussed.

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