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

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dc.creatorMartocchia, Andrea
dc.creatorMatt, Giorgio
dc.creatorKaras, Vladimir
dc.date2002-01-12
dc.date.accessioned2026-07-07T02:02:14Z
dc.date.available2026-07-07T02:02:14Z
dc.descriptionThe 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.
dc.description4 pages, 3 figures. Accepted for publication on A&A Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/0201192
dc.identifierhttp://arxiv.org/abs/astro-ph/0201192
dc.identifierAstron.Astrophys. 383 (2002) L23-L26
dc.identifierdoi:10.1051/0004-6361:20020089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4016
dc.subjectAstrophysics
dc.titleOn the origin of the broad, relativistic iron line of MCG-6-30-15 observed by XMM-Newton
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