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Ionized Disc Models of MCG-6-30-15 | | D.R. Ballantyne
; A.C. Fabian
; S. Vaughan
; | | Date: |
28 Nov 2002 | | Subject: | astro-ph | | Affiliation: | 1,2), A.C. Fabian , S. Vaughan ( IoA, Cambridge CITA, Toronto | | Abstract: | 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. | | Source: | arXiv, astro-ph/0211631 | | Services: | Forum | Review | PDF | Favorites | |
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