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On the origin of the broad, relativistic iron line of MCG-6-30-15 observed by XMM-Newton

Andrea Martocchia·Giorgio Matt·Vladimir Karas
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Abstract

The relativistic iron line profile recently observed by XMM-Newton in the spectrum of the Seyfert 1 galaxy MCG--6-30-15 (Wilms et al., 2001) is discussed in the framework of the lamp-post model. It is shown that the steep disc emissivity, the large line equivalent width and the amount of Compton reflection can be self- consistently reproduced in this scenario.

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Andrea Martocchia, Giorgio Matt, Vladimir Karas. 2002-01-12. On the origin of the broad, relativistic iron line of MCG-6-30-15 observed by XMM-Newton. https://doi.org/10.1051/0004-6361%3A20020089

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