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2002A&A...383L..23M - Astronomy and Astrophysics, volume 383L23-26 (2002/3-1)
On the origin of the broad, relativistic iron line of MCG-6-30-15 observed by XMM-Newton.
MARTOCCHIA A., MATT G. and KARAS V.
Abstract (from CDS):
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., 2001MNRAS.328L..27W) 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.
Abstract Copyright: ∼
Journal keyword(s): relativity - line: profiles - black hole physics - accretion, accretion discs - X-rays: galaxies - individual: MCG-6-30-15
Simbad objects: 1
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