Applicability of the hollow-cone model to pulsars

Details Applicability of the hollow-cone model to pulsars Applicability of the hollow-cone model to pulsars

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..442i&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Oct. 1977, p. 442-445. In Russian.

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2

Pulsar Magnetospheres, Pulsars, Stellar Models, Stellar Radiation, Electromagnetic Pulses, Polarization (Waves), Pulse Duration, Radiant Flux Density

Scientific paper

Predictions based on the hollow-emission-cone model used in describing pulsar magnetospheres are compared with observational data on several pulsars. It is shown that the hollow-cone model cannot explain the presence of more than two components in a pulse profile, the rotation of the plane of polarization of the emission from some pulsars, the ratio between the number of pulsars with two-component and simple pulse profiles at various frequencies, or certain other relations among observed pulsar parameters. Possible alternative models are briefly noted.

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