A model for distortions of polarisation-angle curves in radio pulsars

J. Dyks 1 M. Serylak 2, 3 S. Osłowski 4 L. Saha 1 Lucas Guillemot 5, 6 Ismaël Cognard 5, 6 B. Rudak 1
1 CAMK - Copernicus Astronomical Center of the Polish Academy of Sciences
2 Department of Physics and Astronomy [South Africa]
3 OP - Observatoire de Paris - Site de Paris
4 MPIFR - Max-Planck-Institut für Radioastronomie
5 USN - Unité Scientifique de la Station de Nançay
6 LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace
Abstract : Some radio pulsar profiles (in particular those of millisecond pulsars contain wide emission structures which cover large intervals of pulse phase. Local distortions of an average curve of polarisation angle (PA) can be identified in such profiles, and they are often found to be associated with absorption features or narrow emission components. The features may be interpreted as a convolution of a lateral profile of an emitter with a microscopic radiation pattern of a non-negligible angular extent. We study a model which assumes that such an extended microbeam of the X-mode curvature radiation is spreading the radiation polarised at a fixed position angle within an interval of pulse phase. The model is capable of interpreting the strongly dissimilar polarisation of double notches in PSR B1821-24A (for which we present new polarisation data from the Nancay Radio Telescope) and PSR J0437-4715. It also explains a step-like change in PA observed at the bifurcated trailing component in the profile of J0437-4715. A generic form of the modelled PA distortion is a zigzag-shaped wiggle, which in the presence of the second polarisation mode (O mode) can be magnified or transformed into a W- or U-shaped deflection of a total net PA. The model's efficiency in interpreting dissimilar polarisation effects provides further credence to the stream-based (fan-beam) geometry of pulsar emission. It also suggests that the microbeam width may not always be assumed negligible in comparison with the angular scale of emissivity gradients in the emission region.
Keywords : pulsars: individual: PSR J0437-4715 radiation mechanisms: non-thermal pulsars: individual: PSR B1821-24A pulsars: general
Type de document :
Article dans une revue
Astronomy and Astrophysics - A&A, EDP Sciences, 2016, 593, A83 (14 p.). 〈10.1051/0004-6361/201628516〉
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Soumis le : jeudi 19 janvier 2017 - 11:24:39
Dernière modification le : jeudi 7 février 2019 - 16:07:48
Document(s) archivé(s) le : jeudi 20 avril 2017 - 12:51:53

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J. Dyks, M. Serylak, S. Osłowski, L. Saha, Lucas Guillemot, et al.. A model for distortions of polarisation-angle curves in radio pulsars. Astronomy and Astrophysics - A&A, EDP Sciences, 2016, 593, A83 (14 p.). 〈10.1051/0004-6361/201628516〉. 〈insu-01432989〉

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