Accurate Modelling of Relativistic Iron Lines from Accretion Discs(Session 8 : Key Physical Evidence for BHs)
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概要
- 論文の詳細を見る
Observations of fluorescent iron lines from accreting black holes provide one of the best tests of strong field gravity available to date, and the only current observational tool to probe black hole spacetime. However, the two most widely used models for spectral fitting (diskline, laor) are over a decade old and have significant limitations. We present a new code for calculating these effects which will be incorporated within the XSPEC package.
- 理論物理学刊行会の論文
- 2004-11-15
著者
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Done Chris
Department Of Physics Durham University
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BECKWITH Kris
Department of Physics, University of Durham
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Beckwith Kris
Department Of Physics University Of Durham
関連論文
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- Suzaku Discovery of Absorption Lines from the Black Hole Transient 4U1630-472(Chapter 9. Stellar/Intermediate Mass Black Holes, The Extreme Universe in the Suzaku Era)
- Suzaku observation of two ultraluminous X-ray sources in NGC 1313
- Suzaku Discovery of Iron Absorption Lines in Outburst Spectra of the X-Ray Transient 4U 1630-472
- Understanding of X-Ray Spectra of Black Hole Binaries and Its Application to ULXs(Session 1 : Galactic BH Binaries)
- Spectral Study of GX 339-4 in the Low-Intensity State Observed with Ginga
- Spectral Transitions in X-Ray Binaries(Session 1 : Galactic BH Binaries)
- The Origin of the Soft Excess in High L/L_ AGN(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
- Accurate Modelling of Relativistic Iron Lines from Accretion Discs(Session 8 : Key Physical Evidence for BHs)
- Spectral and Timing Studies of Cyg X-1 in the Low/Hard State with Suzaku
- Understanding of X-Ray Spectra of Black Hole Binaries and Its Application to ULXs(Session 1 : Galactic BH Binaries)
- Spectral Transitions in X-Ray Binaries(Session 1 : Galactic BH Binaries)
- Accurate Modelling of Relativistic Iron Lines from Accretion Discs(Session 8 : Key Physical Evidence for BHs)