Hostname: page-component-76fb5796d-wq484 Total loading time: 0 Render date: 2024-04-26T03:02:44.664Z Has data issue: false hasContentIssue false
  • English
  • Français

Crab Pulsar Radiation Characteristics

Published online by Cambridge University Press:  07 February 2017

R. N. Manchester
R. N. Manchester*
Affiliation:
National Radio Astronomy Observatory, Green Bank, W. V., U.S.A.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It has been suggested that for the Crab pulsar the radio radiation mechanism may be different from that in other pulsars. The principal observations leading to this suggestion are, firstly, the essentially constant position angle of the highly linearly polarised precursor, and secondly, the occasional large increases in intensity of the main pulse.

Type
Session 3
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 209 - 210
Copyright
Copyright © Reidel 1971