Year: 2024
Type: article
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.
Institutions: Commonwealth Scientific and Industrial Research Organisation, Australia Telescope National Facility, University of Manchester, Max Planck Institute for Radio Astronomy, ARC Centre of Excellence for Gravitational Wave Discovery, Swinburne University of Technology, South African Radio Astronomy Observatory, University of Oxford, SKA Observatory, University of the Western Cape
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $3,012
Funders: Magdalen College, University of Oxford, Australian Government, Royal Society, European Commission, National Research Foundation, Swinburne University of Technology, Max-Planck-Gesellschaft, Horizon 2020 Framework Programme, Observatoire de Paris, Université de Recherche Paris Sciences et Lettres, Science and Technology Facilities Council, Australian Research Council, H2020 European Research Council
OpenAlex ID: W4403502388