The shape of pulsar radio beams
arXiv:astro-ph/0010538 · doi:10.1046/j.1365-8711.2001.04146.x
Abstract
Using all available multi-component radio pulse profiles for pulsars with medium to long periods and good polarisation data, we have constructed a two-dimensional image of the mean radio beamshape. This shows a peak near the centre of the beam but is otherwise relatively uniform with only mild enhancements in a few regions. This result supports the patchy-beam model for emission beams in which the mean beam shape represents the properties of the emission mechanism and observed pulse components result from emission sources distributed randomly across the beam.
5 pages, 4 figures. Accepted by MNRAS
References in corpus (1)
Cited by in corpus (27)
- Binary and Millisecond Pulsars
- The FAST Galactic Plane Pulsar Snapshot survey: I. Project design and pulsar discoveries
- A Study of Multi-frequency Polarization Pulse Profiles of Millisecond Pulsars
- Binary and Millisecond Pulsars
- Precession Interpretation of the Isolated Pulsar PSR B1828-11
- An empirical model for the beams of radio pulsars
- Polarization observations of 20 millisecond pulsars
- Binary and Millisecond Pulsars at the New Millennium
- Observations of Non-radial Pulsations in Radio Pulsars
- Gamma-ray and Radio Properties of Six Pulsars Detected by the Fermi Large Area Telescope
- Observations and Modelling of Relativistic Spin Precession in PSR J1141-6545
- A Fan Beam Model for Radio Pulsars. I. Observational Evidence
- The Nature of Coherent Radio Emission from Pulsars
- An Empirical Model for the Radio Emission from Pulsars
- Polarization observations of 100 pulsars at 774 MHz by the Green Bank Telescope
- The Period-Width relationship for radio pulsars revisited
- An inverse Compton scattering (ICS) model of pulsar emission: II. frequency behavior of pulse profiles
- The Polarization of Drifting Subpulses
- Polarization observations of nine southern millisecond pulsars
- Search for a Radio Pulsar in the Remnant of Supernova 1987A
- The High Time Resolution Universe Survey - IX: Polarimetry of long-period pulsars
- Investigating multi-frequency pulse profiles of PSRs B0329+54 and B1642-03 in an inverse Compton scattering (ICS) model
- Modeling the frequency-dependence of radio beams for cone-dominant pulsars
- Structure of pulsar beams: conal versus patchy
- The ratio of profile peak separations as a probe of pulsar radio-beam structure
- Radio emission across the entire rotation phases of pulsars
- Pulsars as Fantastic Objects and Probes