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The X-ray Spectrum Of The Black Hole Candidate Swift J1753.5-0127

The X-ray Spectrum Of The Black Hole Candidate Swift J1753.5-0127

Authors :
Alaa I. Ibrahim
Beike Hiemstra
Mohammed N. Yasein
Mariano Mendez
Paolo Soleri
Reham Mostafa
Tomaso Belloni
Astronomy
Source :
Monthly Notices of the Royal Astronomical Society, 431(3), 2341-2349. Oxford University Press
Publication Year :
2013
Publisher :
arXiv, 2013.

Abstract

We present a spectral analysis of the black hole candidate and X-ray transient source Swift J1753.5 0127 making use of simultaneous observations of XMM-Newton and Rossi X-ray Timing Explorer (RXTE) in 2006, when the source was in outburst. The aim of this paper is to test whether a thermal component due to the accretion disc is present in the X-ray spectrum. We fit the data with a range of spectral models, and we find that for all of these models the fits to the X-ray energy spectra significantly require the addition of the disc black-body component. We also find a broad iron emission line at around 6.5 keV, most likely due to iron in the accretion disc. Our results confirm the existence of a cool inner disc extending near or close to the innermost circular orbit (ISCO).We further discovered broad emission lines of NVII and OVIII at ~ 0.52 keV and 0.65 keV, respectively in the RGS spectrum of Swift J1753.5-0127.<br />Comment: 17 pages, 6 figures, 4 tables, Accepted 2013 February 19 for publication in Monthly Notices of the Royal Astronomical Society Main Journal

Details

ISSN :
00358711
Database :
OpenAIRE
Journal :
Monthly Notices of the Royal Astronomical Society, 431(3), 2341-2349. Oxford University Press
Accession number :
edsair.doi.dedup.....20a7042a29da3d18250452327bf17ae4
Full Text :
https://doi.org/10.48550/arxiv.1302.5882