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- W3106409320 abstract "Context. The number of strong iron Kα line detections in Seyfert AGN is clearly growing in the Chandra, XMM-Newton and Suzaku era. The iron emission lines are broad, some are relativistically blurred. These relativistic disk lines have also been observed for galactic black hole X-ray binaries. Thermal components found in hard spectra were interpreted as an indication for a weak inner cool accretion disk underneath a hot corona." @default.
- W3106409320 created "2020-11-23" @default.
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- W3106409320 date "2011-02-09" @default.
- W3106409320 modified "2023-10-16" @default.
- W3106409320 title "Broad iron emission lines in Seyfert galaxies – re-condensation of gas onto an inner disk below the ADAF?" @default.
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- W3106409320 doi "https://doi.org/10.1051/0004-6361/201015478" @default.
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