A two-component ionized reflection model of MCG-6-30-15
نویسندگان
چکیده
منابع مشابه
A two-component ionized reflection model of MCG–6-30-15
Ionized reflection has often been considered as the explanation for the unusual Fe Kα variability observed in MCG–6-30-15. In this paper, we test this model using a 325 ks observation of MCG–6-30-15 by XMM-Newton and BeppoSAX. The data are fit between 2.5 and 80 keV with the constant density models of Ross & Fabian. The best fit ionized reflection model requires the Fe Kα line to be split into ...
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Ionized reflection is one of the possible mechanisms proposed to explain the small short-timescale variability of the MCG–6-30-15 Fe Kα line. In this contribution, we fit 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 rep...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2003
ISSN: 0035-8711,1365-2966
DOI: 10.1046/j.1365-8711.2003.06533.x