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On the Nature of Magnetars
Published online by Cambridge University Press: 19 July 2016
Abstract
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The electromagnetic fields of magnetodipole radiation can penetrate to the conducting matter of a neutron star crust and create there electric currents and tangential magnetic fields of high magnitude. The solution obtained here has the form of surface magnetic field discontinuities propagating through the crust to the core. This model explains the phenomena of magnetars — Soft Gamma-ray Repeaters and Anomalous X-ray Pulsars.
- Type
- Part 5: Magnetars, Central Compact Objects and Isolated Neutron Stars
- Information
- Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 265 - 266
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
Beskin, V. S., Gurevich, A. V., & Istomin, Ya. N.
1993, Physics of the Pulsar Magnetosphere, (Cambridge: CUP)Google Scholar