Physical properties of the AXP 4U 0142+61 from x-ray spectral analysis

Warning The system is temporarily closed to updates for reporting purpose.

Güver, Tolga and Özel, Feryal and Göğüş, Ersin (2008) Physical properties of the AXP 4U 0142+61 from x-ray spectral analysis. Astrophysical Journal, 675 (2). pp. 1499-1504. ISSN 0004-637x

This is the latest version of this item.

PDF - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader

Official URL: http://dx.doi.org/10.1086/525840


We analyze archival Chandra and XMM-Newton data of 4U 0142+61 within the context of the surface thermal emission and magnetospheric scattering model.We show that the 4U 0142+61 spectrum can be fit very well with this physical model that contains only four parameters. The system parameters can be tightly constrained from the fits, yielding a surface magnetic field strength of B ¼ (4:75 0:02) ; 1014 G, a surface temperature of kT ¼ 0:309 0:001 keV, and a scattering optical depth of a few in the magnetosphere. These values do not vary between observations due to the stability of the source within the window of the observations. The detailed fits yield 2 values that are statistically much better than the traditionally employed blackbody+power-law and two blackbody fits. The spectroscopically measured surface magnetic field strength is higher than, but within, the theoretical uncertainties of the value inferred from the dipole spin-down formula.

Item Type:Article
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
ID Code:10104
Deposited By:Ersin Göğüş
Deposited On:08 Nov 2008 11:49
Last Modified:19 Jul 2019 15:53

Available Versions of this Item

Repository Staff Only: item control page