Iron line profiles in strong gravity
Open Access
- 1 August 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 352 (2), 353-362
- https://doi.org/10.1111/j.1365-2966.2004.07955.x
Abstract
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This publication has 33 references indexed in Scilit:
- The iron line in MCG--6-30-15 from XMM--Newton: evidence for gravitational light bending?Monthly Notices of the Royal Astronomical Society, 2003
- X-ray reflection by photoionized accretion discsMonthly Notices of the Royal Astronomical Society, 2001
- On the meaning of the separation constant in the Kerr metricClassical and Quantum Gravity, 1999
- Line emission from accretion discs around black holes: the analytic approachNew Astronomy, 1998
- Spectral variations of LMC X-3 observed with GINGAThe Astrophysical Journal, 1993
- Application of a general relativistic accretion disk model to LMC X-1, LMC X-3, X1608 - 522, and X1636 - 536The Astrophysical Journal, 1991
- X-ray fluorescence from the inner disc in Cygnus X-1Monthly Notices of the Royal Astronomical Society, 1989
- The effects of redshifts and focusing on the spectrum of an accretion disk around a Kerr black holeThe Astrophysical Journal, 1975
- The Optical Appearance of a Star Orbiting an Extreme Kerr Black HoleThe Astrophysical Journal, 1973
- Global Structure of the Kerr Family of Gravitational FieldsPhysical Review B, 1968