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Frequency dependence of orthogonal polarisation modes in pulsars

J. M. SmitsDepartment of Astrophysics, Radboud University Nijmegen, Nijmegen, The Netherlands e-mail: [email protected]B. W. StappersASTRON, Dwingeloo, The NetherlandsR. T. EdwardsAustralia Telescope National Facility, CSIRO, AustraliaJ. KuijpersDepartment of Astrophysics, Radboud University Nijmegen, Nijmegen, The Netherlands e-mail: [email protected]R. RamachandranDepartment of Astronomy, University of California, Berkeley, USA

2006en

ABI

Annotatsiya

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.

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DOI: 10.1051/0004-6361:20053259

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