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Galaxies 2018, 6(1), 36; doi:10.3390/galaxies6010036

Multi-Wavelength Polarimetry of Isolated Neutron Stars

INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica Milano, via E. Bassini 15, 20133 Milano, Italy
Janusz Gil Institute of Astronomy, University of Zielona Góra, ul. Szafrana 2, 65-516 Zielona Góra, Poland
Received: 29 January 2018 / Revised: 7 March 2018 / Accepted: 9 March 2018 / Published: 13 March 2018
(This article belongs to the Special Issue The Bright Future of Astronomical X-ray Polarimetry)
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Isolated neutron stars are known to be endowed with extreme magnetic fields, whose maximum intensity ranges from 10 12 10 15 G, which permeates their magnetospheres. Their surrounding environment is also strongly magnetized, especially in the compact nebulae powered by the relativistic wind from young neutron stars. The radiation from isolated neutron stars and their surrounding nebulae is, thus, supposed to bring a strong polarization signature. Measuring the neutron star polarization brings important information about the properties of their magnetosphere and of their highly magnetized environment. Being the most numerous class of isolated neutron stars, polarization measurements have been traditionally carried out for radio pulsars, hence in the radio band. In this review, I summarize multi-wavelength linear polarization measurements obtained at wavelengths other than radio both for pulsars and other types of isolated neutron stars and outline future perspectives with the upcoming observing facilities. View Full-Text
Keywords: neutron star; polarimetry; observations neutron star; polarimetry; observations

This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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Mignani, R.P. Multi-Wavelength Polarimetry of Isolated Neutron Stars. Galaxies 2018, 6, 36.

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