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High magnetic field neutron stars and magnetars in binary systems

Published online by Cambridge University Press:  27 February 2023

Sergei B. Popov Open the ORCID record for Sergei B. Popov [Opens in a new window]
Sergei B. Popov*
Affiliation:
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetski pr. 13, 119234, Moscow, Russia email: [email protected]
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Abstract

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Situation with highly magnetized neutron stars in binary systems is not yet certain. On the one hand, all best studied magnetars seem to be isolated objects. On the other, there are many claims based on model-dependent analysis of spin properties or/and luminosity of neutron stars in X-ray binaries in favour of large fields. In addition, there are a few results suggesting a magnetar-like activity of neutron stars in close binary systems. Most of theoretical considerations do not favour even existence, not speaking about active decay, of magnetar-scale fields in neutron stars older than ∼106 yrs. However, alternative scenarios of the field evolution exist. I provide a brief review of theoretical and observational results related to the presence of neutron stars with large magnetic field in binaries and discuss perspectives of future studies.

Keywords

stars: neutronbinaries: closeX-rays: binariesaccretionaccretion disks
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S363: Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution , June 2020 , pp. 61 - 71
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

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