On the origin of the broad, relativistic iron line of MCG-6-30-15 observed by XMM-Newton
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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.
4 pages, 3 figures. Accepted for publication on A&A Letters
4 pages, 3 figures. Accepted for publication on A&A Letters