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| Query : 2000ApJ...543..340T |
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
| Number of rows : 13 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | NAME LMC | G | 05 23 34.6 | -69 45 22 | 0.4 | ~ | 19090 | 0 | ||||
| 2 | PSR B0525-66 | Psr | 05 26 00.7 | -66 04 35 | ~ | 569 | 1 | |||||
| 3 | M 1 | SNR | 05 34 31.8 | +22 01 03 | ~ | 6516 | 1 | |||||
| 4 | V* CM Tau | Psr | 05 34 31.9474694616 | +22 00 52.153698024 | ~ | 5476 | 0 | |||||
| 5 | NAME Vela Pulsar | Psr | 08 35 20.65525 | -45 10 35.1545 | 15.10 | ~ | 2446 | 1 | ||||
| 6 | 2E 2336 | HXB | 10 50 08.93 | -59 53 19.9 | Be | 419 | 0 | |||||
| 7 | 3FHL J1746.2-2852 | LXB | 17 44 33.09 | -28 44 27.0 | ~ | 559 | 0 | |||||
| 8 | PSR J1808-2024 | Psr | 18 08 39.32 | -20 24 40.1 | ~ | 1316 | 2 | |||||
| 9 | SNR G027.3+00.0 | SNR | 18 41 17.8 | -04 56 12 | ~ | 345 | 3 | |||||
| 10 | GBS 1900+14 | gB | 19 07 13 | +09 19.6 | ~ | 906 | 0 | |||||
| 11 | SNR G042.8+00.6 | SNR | 19 07 41.890 | +09 07 17.29 | ~ | 134 | 1 | |||||
| 12 | 2E 4673 | HXB | 23 01 08.14 | +58 52 44.5 | ~ | 673 | 1 | |||||
| 13 | SNR G109.1-01.0 | SNR | 23 01 35 | +58 53.0 | ~ | 362 | 0 |
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