Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-26T04:03:31.385Z Has data issue: false hasContentIssue false
  • English
  • Français

Two-pole Caustic Model for High-energy Radiation from Pulsars — Polarization

Published online by Cambridge University Press:  19 July 2016

Jarosław Dyks ,
Alice K. Harding  and
Bronisław Rudak
Jarosław Dyks
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC, Greenbelt, MD 20771, USA
Alice K. Harding
Affiliation:
Laboratory for High Energy Astrophysics, NASA/GSFC, Greenbelt, MD 20771, USA
Bronisław Rudak
Affiliation:
Nicolaus Copernicus Astronomical Center, 87-100 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.

We present high-energy light curves and polarization properties of pulsars calculated within the recently proposed two-pole caustic model. The results are compared with the optical data for the Crab pulsar and with predictions of other high-energy pulsar models: the polar cap model, and the outer gap model.

Type
Part 8: Pulsar Electrodynamics and Emission Theory
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 373 - 374
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Dyks, J., & Rudak, B. 2003, ApJ, 598, 1201.CrossRefGoogle Scholar
Kanbach, G., Kellner, S., Schrey, F. Z., Steinle, H., Straubmeier, C., & Spruit, H. C. 2003, in Proc. of the SPIE, eds. Iye, M., & Moorwood, A. F. M., 4841, p. 82.CrossRefGoogle Scholar
Kellner, S. 2002, PhD thesis, Technische Universität München.Google Scholar
Romani, R. W., & Yadigaroglu, I.-A. 1995, ApJ, 438, 314.CrossRefGoogle Scholar
Smith, F. G., Jones, D. H. P., Dick, J. S. B., & Pike, C. D. 1988, MNRAS, 233, 305.CrossRefGoogle Scholar