General Relativity studies through X-ray spectroscopy of the Fe (and others) $ K_{α} $ fluorescent lines
Abstract I briefly review in this paper the main observational properties of relativistically broadened X-ray spectral lines in Galactic Black Holes and Active Galactic Nuclei, and the (scanty) estimates of their frequency in the corresponding parent populations. The available measurements allow us...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Guainazzi, Matteo [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2009 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media B.V. 2009 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Springer Netherlands, 1968, 320(2009), 1-3 vom: 24. Feb., Seite 129-134 |
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| Übergeordnetes Werk: |
volume:320 ; year:2009 ; number:1-3 ; day:24 ; month:02 ; pages:129-134 |
| Links: |
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| DOI / URN: |
10.1007/s10509-009-0004-z |
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| 650 | 4 | |a Lines: formation | |
| 650 | 4 | |a Accretion disks | |
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Abstract I briefly review in this paper the main observational properties of relativistically broadened X-ray spectral lines in Galactic Black Holes and Active Galactic Nuclei, and the (scanty) estimates of their frequency in the corresponding parent populations. The available measurements allow us to derive some constraints on the black hole spin and mass, and on the accretion disk geometry and illumination. © Springer Science+Business Media B.V. 2009 |
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Abstract I briefly review in this paper the main observational properties of relativistically broadened X-ray spectral lines in Galactic Black Holes and Active Galactic Nuclei, and the (scanty) estimates of their frequency in the corresponding parent populations. The available measurements allow us to derive some constraints on the black hole spin and mass, and on the accretion disk geometry and illumination. © Springer Science+Business Media B.V. 2009 |
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Abstract I briefly review in this paper the main observational properties of relativistically broadened X-ray spectral lines in Galactic Black Holes and Active Galactic Nuclei, and the (scanty) estimates of their frequency in the corresponding parent populations. The available measurements allow us to derive some constraints on the black hole spin and mass, and on the accretion disk geometry and illumination. © Springer Science+Business Media B.V. 2009 |
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