Broad band X-ray spectrum of KS 1947+300 with BeppoSAX

S. Naik; P. J. Callanan; B. Paul; T. Dotani

doi:10.1086/505555

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Broad band X-ray spectrum of KS 1947+300 with BeppoSAX

S. Naik·P. J. Callanan·B. Paul·T. Dotani

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Abstract

We present results obtained from three BeppoSAX observations of the accretion-powered transient X-ray pulsar KS 1947+300 carried out during the declining phase of its 2000 November -- 2001 June outburst. A detailed spectral study of KS 1947+300 across a wide X-ray band (0.1--100.0 keV) is attempted for the first time here. Timing analysis of the data clearly shows a 18.7 s pulsation in the X-ray light curves in the above energy band. The pulse profile of KS 1947+300 is characterized by a broad peak with sharp rise followed by a narrow dip. The dip in the pulse profile shows a very strong energy dependence. Broad-band pulse-phase-averaged spectroscopy obtained with three of the BeppoSAX instruments shows that the energy spectrum in the 0.1--100 keV energy band has three components, a Comptonized component, a ~0.6 keV blackbody component, and a narrow and weak iron emission line at 6.7 keV with a low column density of material in the line of sight. We place an upper limit on the equivalent width of the iron K_αline at 6.4 keV of ~13 eV (for a width of 100 eV). Assuming a spherical blackbody emitting region and the distance of the source to be 10 kpc, the radius of the emitting region is found to be in the range of 14--22 km, which rules out the inner accretion disk as the soft X-ray emitting region.

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S. Naik, P. J. Callanan, B. Paul, T. Dotani. 2006-05-01. Broad band X-ray spectrum of KS 1947+300 with BeppoSAX. https://doi.org/10.1086/505555

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