The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars

@article{Mereghetti2008TheSC,
  title={The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars},
  author={Sandro Mereghetti},
  journal={The Astronomy and Astrophysics Review},
  year={2008},
  volume={15},
  pages={225-287}
}
  • S. Mereghetti
  • Published 1 April 2008
  • Physics
  • The Astronomy and Astrophysics Review
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… 
Pulsars and Magnetars
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X-ray spectra from magnetar candidates - III. Fitting SGR/AXP soft X-ray emission with non-relativistic Monte Carlo models
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General relativistic neutron stars with twisted magnetosphere
Soft Gamma-Ray Repeaters and Anomalous X-Ray Pulsars are extreme manifestations of the most magnetized neutron stars: magnetars. The phenomenology of their emission and spectral properties strongly
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