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arXiv:astro-ph/0512107 (astro-ph)
[Submitted on 5 Dec 2005 (v1), last revised 25 Jan 2006 (this version, v2)]

Title:Frequency dependence of orthogonal polarisation modes in pulsars

Authors:J.M. Smits, B.W. Stappers, R. T. Edwards, J. Kuijpers, R. Ramachandran
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Abstract: We have carried out a study of the orthogonal polarisation mode behaviour as a function of frequency of 18 pulsars, using average pulsar data from the European Pulsar Network (EPN). Assuming that the radiation consists of two 100% polarised completely orthogonal superposed modes we separated these modes, resulting in average pulse profiles of each mode at multiple frequencies for each pulsar. Furthermore, we studied the frequency dependence of the relative intensity of these modes. We found in many pulsars that the average pulse profiles of the two modes differ in their dependence on frequency. In particular, we found that pulse components that are dominated by one mode tend to increase in intensity with increasing frequency with respect to the rest of the profile.
Comments: 31 pages, 24 figures, 1 table, accepted by A&A; added references in introduction
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0512107
  (or arXiv:astro-ph/0512107v2 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0512107
Related DOI: https://doi.org/10.1051/0004-6361%3A20053259

Submission history

From: J. M. Smits [view email]
[v1] Mon, 5 Dec 2005 14:09:31 UTC (685 KB)
[v2] Wed, 25 Jan 2006 12:51:50 UTC (685 KB)
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