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Wide Beams from Young Pulsars (or One Pole for All)
Published online by Cambridge University Press: 12 April 2016
Abstract
Polarization observations show the existence of a well-defined group of young pulsars with highly linearly polarized mean pulse profiles. Many of these pulsars have interpulses. I suggest that both the main pulse and the interpulse in these pulsars are part of a very wide conal beam emitted along field lines emanating from a single magnetic pole. Such wide beams may be responsible for all interpulse emission.
- Type
- Part 4 Radio Properties
- Information
- International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 193 - 196
- Copyright
- Copyright © Astronomical Society of the Pacific 1996
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