Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-26T04:05:48.306Z Has data issue: false hasContentIssue false
  • English
  • Français

High-frequency Turnover in Pulsar Spectra

Published online by Cambridge University Press:  19 July 2016

J. Kijak  and
O. Maron
J. Kijak
Affiliation:
Institute of Astronomy, University of Zielona Góra, Poland
O. Maron
Affiliation:
Institute of Astronomy, University of Zielona Góra, Poland Max-Planck-Institut für Radioastronomie, Bonn, Germany

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.

Spectra of several pulsars with turnover at unusually high frequencies ∼ 1 GHz are presented. These are relatively young pulsars with DM typically larger than for pulsars showing a low-frequency turnover.

Type
Part 7: Observations of Pulsed Emission
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 339 - 340
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Malofeev, V. M., Gil, J. A., Jessner, A., Malov, I. F., Seiradakis, J. H., Sieber, W., & Wielebinski, R. 1994, A&A, 285, 201.Google Scholar
Maron, O., Kijak, J., Kramer, M., & Wielebinski, R. 2000, A&AS, 147, 195.Google Scholar
Sieber, W. 1973, A&A, 28, 237.Google Scholar
Sieber, W. 2002, in MPE Rep. 278, Neutron Stars, Pulsars and Supernova Remnants, eds. Becker, W., Lesch, H., & Trümper, J., (Garching: MPE), p. 171.Google Scholar