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Multi-Frequency Pulsar Polarimetry at High Frequencies

Published online by Cambridge University Press:  12 April 2016

A. von Hoensbroech  and
K. M. Xilouris
A. von Hoensbroech
Affiliation:
Max-Planck-Institut für Radioastronomies, Bonn, Germany
K. M. Xilouris
Affiliation:
NAIC, Arecibo Observatory, Arecibo, Puerto Rico

Abstract

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A sample of 62 pulsar profiles has been studied with full polarization information at high radio frequencies, aiming at studying the dependency of emission altitude at the deepest layers of pulsar magnetospheres. The emission is consistent with heights ranging between 1-2% of the light-cylinder-radius, while a slight radius-to-frequency mapping is evident.

Type
Part 4 Radio Properties
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 267 - 268
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Blaskiewicz, M., Cordes, J., Wasserman, J. 1991, ApJ, 370, 643 Google Scholar
Hoensbroech, A., Xilouris, K.M. 1996a, A&A, in prep.Google Scholar
Hoensbroech, A., Xilouris, K.M. 1996b, A&A, in prep.Google Scholar
Rankin, J.M., 1993, ApJS, 85, 145 CrossRefGoogle Scholar