The continuum and line spectra of SGR1806-20 bursts

• Published in: Astrophysics and space science Vol. 308; no. 1-4; pp. 43 - 50
• Main Authors: Ibrahim, Alaa I, Parke, William C, Swank, Jean H, Anwer, Hisham, Turolla, Roberto, Zane, Silvia, Hussein, M T, El-Sherbini, T
• Format: Journal Article
• Language: English
• Published: 01.04.2007
• Subjects: Arrays; Bremsstrahlung; Bursts; Centroids; Continuums; Detectors; Emission; Spectral lines; X-rays
• ISSN: 0004-640X; 1572-946X
• DOI: 10.1007/s10509-007-9311-4

The defining property of Soft Gamma Repeaters is the emission of short, bright bursts of X-rays and soft gamma -rays. Here we present the continuum and line spectral properties of a large sample of bursts from SGR1806-20, observed with the Proportional Counter Array (PCA) onboard the Rossi X-ray Timing Explorer (RXTE). Using 10 trail spectral models (5 single and 5 two component models), we find that the burst continua are best fitted by the single component models: cutoff power-law, optically thin bremsstrahlung, and simple power-law. Time resolved spectroscopy show that there are two absorption lines at 5 keV and 20 keV in some bursts. The lines are relatively narrow with 90% upper limit on the line widths of 0.5-1.5 keV for the 5keV feature and 1-3 keV for the 20 keV feature. Both lines have considerable equivalent width of 330-850 eV for the 5keV feature and 780-2590 eV for the 20keV feature. We examined whether theses spectral lines are dependent upon the choice of a particular continuum model and find no such dependence. Besides, we find that the 5keV feature is pronounced with high confidence in the cumulative joint spectrum of the entire burst sample, both in the individual detectors of the PCA and in the co-added detectors spectrum. We confront the features against possible instrumental effects and find that none can account for the observed line properties. The two features do not seem to be connected to the same physical mechanism because (1) they do not always occur simultaneously, (2) while the 5keV feature occurs at about the same energy, the 20keV line centroid varies significantly from burst to burst over the range 18-22keV, and (3) the centroid of the lines shows anti-correlated red/blue shifts. The transient appearance of the features in the individual bursts and in portions of the same burst, together with the spectral evolution seen in some bursts point to a complex emission mechanism that requires further investigation.