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2000ApJ...543..340T - Astrophys. J., 543, 340-350 (2000/November-1)
Physical mechanisms for the variable spin-down and light curve of Sgr 1900+14.
THOMPSON C., DUNCAN R.C., WOODS P.M., KOUVELIOTOU C., FINGER M.H. and VAN PARADIJS J.
Abstract (from CDS):
The change in the persistent X-ray light curve following the August 27 event is ascribed to continued particle heating in the active region of that outburst. The enhanced X-ray output can be powered by a steady current flowing through the magnetosphere, induced by the twisting motion of the crust. The long-term rate of spin-down appears to be accelerated with respect to a simple magnetic dipole torque. Accelerated spin-down of a seismically active magnetar will occur when its persistent output of Alfvén waves and particles exceeds its spin-down luminosity or if particle flows modulate the ratio of conduction to displacement currents in the outer magnetosphere. We suggest that SGRs experience some episodes of relative inactivity, with diminished P{dot}, and that such inactive magnetars are observed as anomalous X-ray pulsars (AXPs). The reappearance of persistent X-ray emission from SGR 1900+14 within one day of the August 27 event provides strong evidence that the persistent emission is not powered by accretion.
Abstract Copyright: ∼
Journal keyword(s): Stars: Pulsars: General - Stars: Individual: Alphanumeric: SGR 1900+14 - X-Rays: Bursts
Simbad objects: 13
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