The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars
Abstract:
Two classes of X-ray pulsars, the anomalous X-ray pulsars and the soft gamma-ray repeaters, have been recognized in the last decade as the most promising candidates for being magnetars: isolated neutron stars powered by magnetic energy. I review the observational properties of these objects, focussing on the most recent results, and their interpretation in the magnetar model. Alternative explanations, in particular those based on accretion from residual disks, are also considered. The possible relations between these sources and other classes of neutron stars and astrophysical objects are also discussed.read more
Citations
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A Broadband Emission Model of Magnetar Wind Nebulae
TL;DR: In this paper, a broadband emission model of magnetar wind nebulae (MWNe) was constructed for the first time and applied to the MWN around the youngest magnetar 1E 1547.0-5408 that has the largest spin-down power.
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Relativistic expansion of magnetic loops at the self‐similar stage – II. Magnetized outflows interacting with the ambient plasma
TL;DR: In this paper, the authors obtained self-similar solutions of relativistically expanding magnetic loops by assuming axisymmetry and a purely radial flow, and they used the analytical solutions as the initial condition and the inner boundary conditions.
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Constraints on physics of neutron stars from X-ray observations
TL;DR: In this paper, the authors summarize some constraints on the physics of neutron stars arising from X-ray observations of the surfaces of the neutron stars, focusing on using models of low-magnetic-field neutron star atmospheres to interpret their Xray spectra.
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On the Polarization Properties of Magnetar Giant Flare Pulsating Tails
TL;DR: In this paper, the atmospheric structure of the trapped fireball and the polarization properties of a trapped fireball were derived from a closed-field-line region in the magnetosphere of a soft gamma-ray repeater.
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Modified Fermi Energy of Electrons in a Superhigh Magnetic Field
TL;DR: In this paper, the electron Landau-level stability and its influence on the electron Fermi energy were investigated in the circumstance of magnetars, which are powered by magnetic field energy.
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An X-ray pulsar with a superstrong magnetic field in the soft γ-ray repeater SGR1806 − 20
Chryssa Kouveliotou,Chryssa Kouveliotou,S. Dieters,S. Dieters,Tod E. Strohmayer,Tod E. Strohmayer,J. van Paradijs,Gerald J. Fishman,Charles A. Meegan,Kevin Hurley,Jefferson M. Kommers,Ian Smith,Dale A. Frail,Toshio Murakami +13 more
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