Statistics of relativistically broadened Fe Kα lines in AGN
- 28 November 2006
- journal article
- research article
- Published by Wiley in Astronomische Nachrichten
- Vol. 327 (10) , 1032-1038
- https://doi.org/10.1002/asna.200610687
Abstract
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This publication has 24 references indexed in Scilit:
- The nature and origin of Seyfert warm absorbersAstronomy & Astrophysics, 2005
- Long-term spectral changes in the partial-covering candidate narrow-line Seyfert 1 galaxy 1H 0707-495Monthly Notices of the Royal Astronomical Society, 2004
- X-ray reflection in the narrow-line Seyfert 1 galaxy 1H 0707-495Monthly Notices of the Royal Astronomical Society, 2004
- An Extended Scheme for Fitting X‐Ray Data with Accretion Disk Spectra in the Strong Gravity RegimeThe Astrophysical Journal Supplement Series, 2004
- Multiwavelength studies of the Seyfert 1 galaxy NGC 7469 II. X-ray and UV observations with XMM-NewtonAstronomy & Astrophysics, 2003
- Simultaneous XMM-Newton and BeppoSAX observation of the Seyfert I galaxy IC 4329AAstronomy & Astrophysics, 2001
- The X-ray Baldwin effectThe Astrophysical Journal, 1993
- Line profiles from a disk around a rotating black holeThe Astrophysical Journal, 1991
- X-ray fluorescence from the inner disc in Cygnus X-1Monthly Notices of the Royal Astronomical Society, 1989
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989