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
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.
منابع مشابه
ar X iv : a st ro - p h / 97 07 20 2 v 1 1 7 Ju l 1 99 7 Broad - band continuum and variability of NGC 5548
We analyze a composite broad-band optical/UV/Xγ-ray spectrum of the Seyfert 1 galaxy NGC 5548. The spectrum consists of an average of simultaneous optical/IUE/Ginga observations accompanied by ROSAT and GRO/OSSE data from non-simultaneous observations. We show that the broad-band continuum is inconsistent with simple disk models extending to the soft X-rays. Instead, the soft-excess is well des...
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