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Long term spectral variability in the Soft Gamma-ray Repeater SGR 1900+14

A. Tiengo·P. Esposito·S. Mereghetti·L. Sidoli·D. Goetz·M. Feroci·R. Turolla·S. Zane·G. L. Israel·L. Stella·P. Woods
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Abstract

We present a systematic analysis of all the BeppoSAX data of SGR1900+14. The observations spanning five years show that the source was brighter than usual on two occasions: ~20 days after the August 1998 giant flare and during the 10^5 s long X-ray afterglow following the April 2001 intermediate flare. In the latter case, we explore the possibility of describing the observed short term spectral evolution only with a change of the temperature of the blackbody component. In the only BeppoSAX observation performed before the giant flare, the spectrum of the SGR1900+14 persistent emission was significantly harder and detected also above 10 keV with the PDS instrument. In the last BeppoSAX observation (April 2002) the flux was at least a factor 1.2 below the historical level, suggesting that the source was entering a quiescent period.

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A. Tiengo, P. Esposito, S. Mereghetti, L. Sidoli, D. Goetz, M. Feroci, R. Turolla, S. Zane, G. L. Israel, L. Stella, P. Woods. 2006-09-12. Long term spectral variability in the Soft Gamma-ray Repeater SGR 1900+14. https://doi.org/10.1007/s10509-007-9300-7

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