Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz

We present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, observed at 1.4 and 3.1 GHz. Absolute PAs are obtained at each frequency, permitting a measurement of the difference in the profiles. By doing this, we obtain more precise rotation measure (RM) values...

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Main Authors: Karastergiou, A, Johnston, S
Format: Journal article
Published: 2005
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author Karastergiou, A
Johnston, S
author_facet Karastergiou, A
Johnston, S
author_sort Karastergiou, A
collection OXFORD
description We present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, observed at 1.4 and 3.1 GHz. Absolute PAs are obtained at each frequency, permitting a measurement of the difference in the profiles. By doing this, we obtain more precise rotation measure (RM) values for some of the pulsars in the current catalogue. We find that, apart from RM corrections, there are small, pulse longitude dependent differences in PA with frequency. Such differences go beyond the interpretation of a geometrical origin. We describe in detail the PA evolution between the two frequencies and discuss possible causes, such as orthogonal and non-orthogonal polarisation modes of emission. We also use the PA and total power profiles to estimate the difference in emission height at which the two frequencies originate. In our data sample, there are changes in the relative strengths of different pulse components, especially overlapping linearly polarised components, which coincide with intrinsic changes of the PA profile, resulting in interesting PA differences between the two frequencies.
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spelling oxford-uuid:cd760ca2-a977-4bc2-be2f-405bc7be7fca2022-03-27T07:28:52ZAbsolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHzJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:cd760ca2-a977-4bc2-be2f-405bc7be7fcaSymplectic Elements at Oxford2005Karastergiou, AJohnston, SWe present here a direct comparison of the polarisation position angle (PA) profiles of 17 pulsars, observed at 1.4 and 3.1 GHz. Absolute PAs are obtained at each frequency, permitting a measurement of the difference in the profiles. By doing this, we obtain more precise rotation measure (RM) values for some of the pulsars in the current catalogue. We find that, apart from RM corrections, there are small, pulse longitude dependent differences in PA with frequency. Such differences go beyond the interpretation of a geometrical origin. We describe in detail the PA evolution between the two frequencies and discuss possible causes, such as orthogonal and non-orthogonal polarisation modes of emission. We also use the PA and total power profiles to estimate the difference in emission height at which the two frequencies originate. In our data sample, there are changes in the relative strengths of different pulse components, especially overlapping linearly polarised components, which coincide with intrinsic changes of the PA profile, resulting in interesting PA differences between the two frequencies.
spellingShingle Karastergiou, A
Johnston, S
Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
title Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
title_full Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
title_fullStr Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
title_full_unstemmed Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
title_short Absolute polarisation position angle profiles of southern pulsars at 1.4 and 3.1 GHz
title_sort absolute polarisation position angle profiles of southern pulsars at 1 4 and 3 1 ghz
work_keys_str_mv AT karastergioua absolutepolarisationpositionangleprofilesofsouthernpulsarsat14and31ghz
AT johnstons absolutepolarisationpositionangleprofilesofsouthernpulsarsat14and31ghz