Testing the Kerr nature of black hole candidates using iron line reverberation mapping in the Cardoso-Pani-Rico framework
The iron Kα line commonly observed in the x-ray spectrum of black hole candidates is produced by x-ray fluorescence of the inner accretion disk. This line can potentially be quite a powerful tool to probe the spacetime geometry around these objects and test the Kerr black hole hypothesis. In a previ...
| Asıl Yazarlar: | , , |
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| Diğer Yazarlar: | |
| Materyal Türü: | Makale |
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American Physical Society
2018
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| Online Erişim: | http://hdl.handle.net/1721.1/116627 |