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

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. [CITE]) 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