MeerKAT observations of pair-plasma induced birefringence in the double pulsar eclipses

ABSTRACT PSR J0737−3039A/B is unique among double neutron star systems. Its near-perfect edge-on orbit causes the fast spinning pulsar A to be eclipsed by the magnetic field of the slow spinning pulsar B. Using high-sensitivity MeerKAT radio observations combined with updated constraints on the system geometry, we studied the impact of these eclipses on the incident polarization properties of pulsar A. Averaging light curves together after correcting for the rotation of pulsar B revealed enormous amounts of circular polarization and rapid changes in the linear polarization position angle, which occur at phases where emission from pulsar A is partially transmitted through the magnetosphere of pulsar B. These behaviours confirm that the eclipse mechanism is the result of synchrotron absorption in a relativistic pair-plasma confined to the closed-field region of pulsar B’s truncated dipolar magnetic field. We demonstrate that changes in circular polarization handedness throughout the eclipses are directly tied to the average line of sight magnetic field direction of pulsar B, from which we unambiguously determine the complete magnetic and viewing geometry of the pulsar.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-10-17
DOI
https://doi.org/10.1093/mnras/stae2386
Citations
2
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.66

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article

MeerKAT observations of pair-plasma induced birefringence in the double pulsar eclipses

Sarah Buchner, M. Krämer, Norbert Wex, R. M. Shannon et al.
2 citations
Monthly Notices of the Royal Astronomical Society
Stellar, planetary, and galactic studies
0.66
article

MeerKAT observations of pair-plasma induced birefringence in the double pulsar eclipses

Sarah Buchner, M. Krämer, Norbert Wex, R. M. Shannon, L S Oswald, Daniel J. Reardon, R. P. Breton, F. Camilo, M. Serylak, S. Johnston, V. Venkatraman Krishnan, M. Bailes, M. E. Lower
article en
2 citations

Abstract

ABSTRACT PSR J0737−3039A/B is unique among double neutron star systems. Its near-perfect edge-on orbit causes the fast spinning pulsar A to be eclipsed by the magnetic field of the slow spinning pulsar B. Using high-sensitivity MeerKAT radio observations combined with updated constraints on the system geometry, we studied the impact of these eclipses on the incident polarization properties of pulsar A. Averaging light curves together after correcting for the rotation of pulsar B revealed enormous amounts of circular polarization and rapid changes in the linear polarization position angle, which occur at phases where emission from pulsar A is partially transmitted through the magnetosphere of pulsar B. These behaviours confirm that the eclipse mechanism is the result of synchrotron absorption in a relativistic pair-plasma confined to the closed-field region of pulsar B’s truncated dipolar magnetic field. We demonstrate that changes in circular polarization handedness throughout the eclipses are directly tied to the average line of sight magnetic field direction of pulsar B, from which we unambiguously determine the complete magnetic and viewing geometry of the pulsar.

Monthly Notices of the Royal Astronomical SocietyVol. 534(4)
Commonwealth Scientific and Industrial Research Organisation (AU), Australia Telescope National Facility (AU), Northeast Catholic College (US), University of Manchester (GB), University of Oxford (GB), SKA Observatory (GB), South African Radio Astronomy Observatory (ZA), ARC Centre of Excellence for Gravitational Wave Discovery (AU), Max Planck Institute for Radio Astronomy (DE), Swinburne University of Technology (AU), University of the Western Cape (ZA)
Australian Government, Royal Society, European Commission, National Research Foundation, Swinburne University of Technology, Max-Planck-Gesellschaft, Horizon 2020 Framework Programme, Science and Technology Facilities Council, Australian Research Council, H2020 European Research Council
Openalex Percentile: Top 27%
Stellar, planetary, and galactic studies
0.66
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