ar X iv : a st ro - p h / 97 10 18 3 v 1 1 6 O ct 1 99 7 A MODEL OF THE BROAD - BAND CONTINUUM OF NGC 5548

نویسنده

  • P. MAGDZIARZ
چکیده

We discuss a model of the central source in Seyfert 1 galaxy NGC 5548. The model assumes a three phase disk structure consisting of a cold outer disk, a hot central disk constituting a Comptonizing X/γ source, and an intermediate unstable and complex phase emitting a soft excess component. The model qualitatively explains broad-band spectrum and variability behavior assuming that the soft excess contributes significantly to the continuum emission and drives variability by geometrical changes of the intermediate disk zone.

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تاریخ انتشار 1997