A Chandra Survey of Fluorescence Fe Lines in X-ray Binaries at High Resolution
Fe K line fluorescence is commonly observed in the X-ray spectra of many X-ray binaries (XRBs) and represents a fundamental tool to investigate the material surrounding the X-ray source. In this paper, we present a comprehensive survey of 41 XRBs (10 HMXBs and 31 LMXBs) with Chandra with specific em...
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Veröffentlicht in: | The Astrophysical journal 2010-06, Vol.715 (2), p.947-947 |
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Sprache: | eng |
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Zusammenfassung: | Fe K line fluorescence is commonly observed in the X-ray spectra of many X-ray binaries (XRBs) and represents a fundamental tool to investigate the material surrounding the X-ray source. In this paper, we present a comprehensive survey of 41 XRBs (10 HMXBs and 31 LMXBs) with Chandra with specific emphasis on the Fe K region and the narrow Fe K{alpha} line, at the highest resolution possible. We find that (1) the Fe K{alpha} line is always centered at {lambda} = 1.9387 {+-} 0.0016 A, compatible with Fe I up to Fe X; we detect no shifts to higher ionization states nor any difference between high mass X-ray binaries (HMXBs) and low mass X-ray binaries (LMXBs). (2) The line is very narrow, with FWHM { |
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ISSN: | 0004-637X 1538-4357 |
DOI: | 10.1088/0004-637X/715/2/947 |