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Chinese Journal of Astronomy and Astrophysics, 2006
A brief review of known models for the description of Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Repeaters (SGRs) is given. A new model is proposed to explain the main properties of these objects and radio pulsars with long periods on the base of the conception of drift waves in the vicinity of the light cylinder of the neutron star with the ...
I. F Malov, G. Z Machabeli
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A brief review of known models for the description of Anomalous X-ray Pulsars (AXPs) and Soft Gamma-Repeaters (SGRs) is given. A new model is proposed to explain the main properties of these objects and radio pulsars with long periods on the base of the conception of drift waves in the vicinity of the light cylinder of the neutron star with the ...
I. F Malov, G. Z Machabeli
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Physics of Particles and Nuclei, 2019
Soft repeating gamma-ray (SGR) bursts are considered as magnetoemission of crusts of magnetars (ultramagnetized neutron stars). It is shown that all the observations of such bursts can be described and systematized within a randomly jumping interacting moments model including quantum fluctuations and internuclear interaction in an inhomogeneous medium.
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Soft repeating gamma-ray (SGR) bursts are considered as magnetoemission of crusts of magnetars (ultramagnetized neutron stars). It is shown that all the observations of such bursts can be described and systematized within a randomly jumping interacting moments model including quantum fluctuations and internuclear interaction in an inhomogeneous medium.
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Astronomische Nachrichten, 1999
The discovery of long periods and high period derivatives in soft gamma-ray repeaters (SGRs) over the past year has raised the possibility that magnetars, neutron stars having magnetic fields above 1014 G, may be real astrophysical objects. Magnetars are possibly the first astrophysical sources to derive their primary radiation power from magnetic ...
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The discovery of long periods and high period derivatives in soft gamma-ray repeaters (SGRs) over the past year has raised the possibility that magnetars, neutron stars having magnetic fields above 1014 G, may be real astrophysical objects. Magnetars are possibly the first astrophysical sources to derive their primary radiation power from magnetic ...
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Rotating vector model for magnetars
Monthly Notices of the Royal Astronomical Society, 2021H Tong, H G Wang, P F Wang
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Testing the fossil field hypothesis: could strongly magnetized OB stars produce all known magnetars?
Monthly Notices of the Royal Astronomical Society, 2021Alexander Kholtygin +2 more
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The early evolution of magnetar rotation – I. Slowly rotating ‘normal’ magnetars
Monthly Notices of the Royal Astronomical Society, 2022Matthew S B Coleman +2 more
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Modelling spin evolution of magnetars
Monthly Notices of the Royal Astronomical Society, 2021Thomas Tauris
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