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• W2138831523 abstract "We report the results of an XMM-Newton observation of the persistent X–ray source 1E 1743.1–2843, located in the Galactic Center (GC) direction. We determine the position of the source at , (with an uncertainty of 1.5″), which is the most accurate to date, and will enable cross-identifications at other wavelengths. The source was bright during this observation ( erg s-1 for a power-law continuum), with no significant variability. We propose that 1E 1743.1–2843 may be explained in terms of a black hole candidate in a low/hard state. There is an indication that the source exhibits different states from a comparison of our results with previous observations (e.g., ART-P, BeppoSAX). However, the present spectral analysis does not rule out the hypothesis of a neutron star low-mass X-ray binary as suggested previously. If 1E 1743.1–2843 is actually located in the GC region, we might expect to observe significant 6.4 keV fluorescent iron line emission from nearby molecular clouds (e.g., GCM+0.25+0.01)." @default.
• W2138831523 created "2016-06-24" @default.
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• W2138831523 date "2003-07-01" @default.
• W2138831523 modified "2023-10-01" @default.
• W2138831523 title "$vec{XMM}$-$vec{Newton}$ study of the persistent X-ray source 1E 1743.1–2843 located in the Galactic Center direction" @default.
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• W2138831523 doi "https://doi.org/10.1051/0004-6361:20030770" @default.
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