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Origin of magnetars in binary systems

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arxiv 1507.08192 v1 pith:57ENW5IE submitted 2015-07-28 astro-ph.HE

S.B. Popov (Sternberg Astronomical Institute , Russia) This is my paper · ORCID
classification astro-ph.HE
keywords magnetarsbinarycandidatesfieldformationmagneticmodelsproposed
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I review several scenarios of magnetar formation in binary systems via spin-up of a progenitor due to interaction with its companion. Mostly, these evolutionary channels lead to formation of isolated magnetars, and indeed, all well-established sources of this class are single objects. However, some binaries can survive, and several candidates to accreting magnetars have been proposed. I discuss this issue, and conclude that new accretion models can explain properties of the proposed candidates without large magnetic field in correspondence with models of magnetic field evolution.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Radiative Back-Reaction on Charged Particle Motion in the Dipole Magnetosphere of Neutron Stars

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    Radiative back-reaction makes charged particles under an attractive Lorentz force fall onto a magnetized neutron star, while under a repulsive force they either widen their orbits or fall, depending on the starting latitude.

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