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A New Model of “Magnetar”

Published online by Cambridge University Press:  19 July 2016

I. F. Malov ,
G. Z. Machabeli  and
V. M. Malofeev
I. F. Malov
Affiliation:
Lebedev Physical Institute, Moscow, Russia
G. Z. Machabeli
Affiliation:
Abastumani Astrophysical Observatory, Abastumani, Georgia
V. M. Malofeev
Affiliation:
Lebedev Physical Institute, Moscow, Russia

Abstract

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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 

References

Carlini, A., & Treves, A. 1989, A&A, 215, 283.Google Scholar
Duncan, R. C., & Thompson, C. 1992, ApJ, 392, L9.Google Scholar
Israel, G. L., Mereghetti, S., & Stella, L. 1994, ApJ, 433, L25.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., & Melikidze, G. I. 1987, Aust. J. Phys., 44, 573.Google Scholar
Mereghetti, S., & Stella, L. 1995, ApJ, 442, L17.Google Scholar
Usov, V. V. 1993, ApJ, 410, 763.CrossRefGoogle Scholar