Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-26T06:46:33.375Z Has data issue: false hasContentIssue false
  • English
  • Français

Model of pulse separation in the gamma light curve of the Vela pulsar

Published online by Cambridge University Press:  12 April 2016

Jaroslaw Dyks  and
Bronislaw Rudak
Jaroslaw Dyks
Affiliation:
N. Copernicus Astronomical Center, Rabiańska 8, 87100 Toruń, Poland
Bronislaw Rudak
Affiliation:
N. Copernicus Astronomical Center, Rabiańska 8, 87100 Toruń, Poland

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.

Within the framework of a single polar cap model we calculate the energy dependence of phase separation between two peaks in the gamma-ray lightcurve of the Vela pulsar. Results are confronted with EGRET data (Kanbach 1999).

Type
Part 6. Emission and Plasma Theory
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 433 - 434
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Daugherty, J.K., Harding, A.K. 1982, ApJ, 252, 337 Google Scholar
Kanbach, G. 1999, in Proc. of 3rd INTEGRAL Workshop, in pressGoogle Scholar
Miyazaki, J., Takahara, F. 1997, MNRAS, 290, 49 Google Scholar