Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-26T04:33:44.045Z Has data issue: false hasContentIssue false
  • English
  • Français

Single Pulse Analysis of the Core-Dominated Pulsar B0611+22

Published online by Cambridge University Press:  12 April 2016

Jeffrey S. Kern
Jeffrey S. Kern*
Affiliation:
Department of Physics, New Mexico Institute of Mining and Technology, Socorro NM 87801USA: [email protected]

Abstract

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.

Single pulse studies of pulsar radio emission provide a window into the time dependent behavior of the radio loud region. I have analyzed a series of precision polarimetric observations of pulsar B0611+22 to determine the geometry of the emission region. The observations are consistent with a central core emission region, and a periodically present conal component. This identification leads to the surprising result that all emission is from the leading half of the polar cap.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 175 - 176
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Goldreich, P. & Julian, W.H. 1969, ApJ, 157, 869 CrossRefGoogle Scholar