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A New Model of “Magnetar”
Published online by Cambridge University Press: 19 July 2016
Abstract
A new model is proposed to explain the main properties of anomalous X-ray pulsars and soft gamma-ray repeaters, in terms of drift waves in the vicinity of the light cylinder of a neutron star with a surface magnetic field ∼ 1012 G.
- 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. 271 - 272
- Copyright
- Copyright © Astronomical Society of the Pacific 2004