Ionized Disc Models of MCG-6-30-15
| dc.creator | Ballantyne, D. R. | |
| dc.creator | Fabian, A. C. | |
| dc.creator | Vaughan, S. | |
| dc.date | 2002-11-28 | |
| dc.date.accessioned | 2026-07-07T02:06:36Z | |
| dc.date.available | 2026-07-07T02:06:36Z | |
| dc.description | Ionized reflection is one of the possible mechanisms proposed to explain the small short-timescale variability of the MCG-6-30-15 Fe K line. In this contribution, we show fits of the Ross & Fabian ionized reflection models to the 325 ks XMM-Newton observation of MCG--6-30-15. It is found that the spectrum above 2.5 keV can be fitted with a combination of an ionized reflector from 5 r_g and a neutral reprocessor beyond about 70 r_g. The ionization parameter of the inner reflector increases as the source brightens. | |
| dc.description | 2 pages, 1 figure. To be published in "Active Galactic Nuclei: from Central Engine to Host Galaxy", ed. S. Collin, F. Combes, and I. Shlosman | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0211631 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0211631 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5418 | |
| dc.subject | Astrophysics | |
| dc.title | Ionized Disc Models of MCG-6-30-15 | |
| dc.type | text |