On the x-ray outbursts of transient anomalous x-ray pulsars and soft gamma-ray repeaters

Çalışkan, Şirin and Ertan, Ünal (2012) On the x-ray outbursts of transient anomalous x-ray pulsars and soft gamma-ray repeaters. Astrophysical Journal, 758 (2). ISSN 0004-637X (Print) 1538-4357 (Online)

PDF (This is a RoMEO green journal -- author can archive publisher's version/PDF) - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader

Official URL: http://dx.doi.org/10.1088/0004-637X/758/2/98


We show that the X-ray outburst light curves of four transient anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs), namely, XTE J1810–197, SGR 0501+4516, SGR 1627–41, and CXOU J164710.2–455216, can be produced by the fallback disk model that was also applied to the outburst light curves of persistent AXPs and SGRs in our earlier work. The model solves the diffusion equation for the relaxation of a disk that has been pushed back by a soft gamma-ray burst. The sets of main disk parameters used for these transient sources are very similar to each other and to those employed in our earlier models of persistent AXPs and SGRs. There is a characteristic difference between the X-ray outburst light curves of transient and persistent sources. This can be explained by the differences in the disk surface density profiles of the transient and persistent sources in quiescence indicated by their quiescent X-ray luminosities. Our results imply that a viscous disk instability operating at a critical temperature in the range of ~1300-2800 K is a common property of all fallback disks around AXPs and SGRs. The effect of the instability is more pronounced and starts earlier for the sources with lower quiescent luminosities, which leads to the observable differences in the X-ray enhancement light curves of transient and persistent sources. A single active disk model with the same basic disk parameters can account for the enhancement phases of both transient and persistent AXPs and SGRs. We also present a detailed parameter study to show the effects of disk parameters on the evolution of the X-ray luminosity of AXPs and SGRs in the X-ray enhancement phases.

Item Type:Article
Additional Information:Article Number: 98
Uncontrolled Keywords:accretion, accretion disks; pulsars: individual (AXPs); stars: neutron; X-rays: bursts
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
ID Code:19819
Deposited By:Ünal Ertan
Deposited On:20 Oct 2012 15:46
Last Modified:31 Jul 2019 12:18

Repository Staff Only: item control page