Radio polarization measurements from RRAT J1819-1458

We present the first polarization measurements of the radio emission from RRAT J1819-1458. Our observations, conducted in parallel to regular timing sessions, have yielded a small number of bright and polarized pulses. The polarization characteristics and integrated profile resemble those of normal...

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Main Authors: Karastergiou, A., Hotan, Aidan, van Straten, W., McLaughlin, M., Ord, S.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2009
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/9853
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author Karastergiou, A.
Hotan, Aidan
van Straten, W.
McLaughlin, M.
Ord, S.
author_facet Karastergiou, A.
Hotan, Aidan
van Straten, W.
McLaughlin, M.
Ord, S.
author_sort Karastergiou, A.
building Curtin Institutional Repository
collection Online Access
description We present the first polarization measurements of the radio emission from RRAT J1819-1458. Our observations, conducted in parallel to regular timing sessions, have yielded a small number of bright and polarized pulses. The polarization characteristics and integrated profile resemble those of normal pulsars with average spin-down energy E: moderate to low linear polarization in the integrated profile despite relatively high polarization in the individual pulses. On average, a small degree of circular polarization is also observed. The polarization position angle (PA) executes a remarkably smooth, steep S-shaped curve, interrupted by two orthogonal jumps. Based on the shape of the PA swing, we place some constraints on the emission geometry. We compare these polarization properties to those of other radio-emitting neutron star populations, including young pulsars, pulsars with a high surface magnetic field and radio-emitting magnetars. From the polarization measurements, the Faraday rotation measure of this rotation radio transient is derived.
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institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T06:27:24Z
publishDate 2009
publisher Wiley-Blackwell Publishing Ltd.
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spelling curtin-20.500.11937-98532017-09-13T16:01:58Z Radio polarization measurements from RRAT J1819-1458 Karastergiou, A. Hotan, Aidan van Straten, W. McLaughlin, M. Ord, S. polarization J1819-1458 individual pulsars We present the first polarization measurements of the radio emission from RRAT J1819-1458. Our observations, conducted in parallel to regular timing sessions, have yielded a small number of bright and polarized pulses. The polarization characteristics and integrated profile resemble those of normal pulsars with average spin-down energy E: moderate to low linear polarization in the integrated profile despite relatively high polarization in the individual pulses. On average, a small degree of circular polarization is also observed. The polarization position angle (PA) executes a remarkably smooth, steep S-shaped curve, interrupted by two orthogonal jumps. Based on the shape of the PA swing, we place some constraints on the emission geometry. We compare these polarization properties to those of other radio-emitting neutron star populations, including young pulsars, pulsars with a high surface magnetic field and radio-emitting magnetars. From the polarization measurements, the Faraday rotation measure of this rotation radio transient is derived. 2009 Journal Article http://hdl.handle.net/20.500.11937/9853 10.1111/j.1745-3933.2009.00671.x Wiley-Blackwell Publishing Ltd. unknown
spellingShingle polarization
J1819-1458
individual
pulsars
Karastergiou, A.
Hotan, Aidan
van Straten, W.
McLaughlin, M.
Ord, S.
Radio polarization measurements from RRAT J1819-1458
title Radio polarization measurements from RRAT J1819-1458
title_full Radio polarization measurements from RRAT J1819-1458
title_fullStr Radio polarization measurements from RRAT J1819-1458
title_full_unstemmed Radio polarization measurements from RRAT J1819-1458
title_short Radio polarization measurements from RRAT J1819-1458
title_sort radio polarization measurements from rrat j1819-1458
topic polarization
J1819-1458
individual
pulsars
url http://hdl.handle.net/20.500.11937/9853