[ITAL]ASCA[/ITAL] Observation of the Quiescent X-Ray Counterpart to SGR 1627−41

K. Hurley, Tod E. Strohmayer, P. Li, C. Kouveliotou, P. M. Woods, J. van Paradijs, T. Murakami, D. H. Hartmann, I. A. Smith, Masaki Ando,

The Astrophysical Journal · 2000 · 20 citations · 12 references

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Abstract

We present a 2-10 keV ASCA observation of the field around the soft gamma repeater SGR 1627-41. A quiescent X-ray source, whose position is consistent both with that of a recently discovered BeppoSAX X-ray source and with the Interplanetary Network localization for this soft gamma repeater, was detected in this observation. In 2-10 keV X-rays, the spectrum of the X-ray source may be fit equally well by a power-law, blackbody, or bremsstrahlung function, with unabsorbed flux approximately 5x10-12 ergs cm-2 s-1. We do not confirm a continuation of a fading trend in the flux, and we find no evidence for periodicity, both of which were noted in the earlier BeppoSAX observations.

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