A Model of the Variable Optical, Ultraviolet, and X-ray Continuum of NGC 5548

Details A Model of the Variable Optical, Ultraviolet, and X-ray Continuum of NGC 5548 A Model of the Variable Optical, Ultraviolet, and X-ray Continuum of NGC 5548

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.3614b&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #36.14; Bulletin of the American Astronomical Society, Vol. 30, p.864

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a detailed broadband spectral model of the continuum emission in the Seyfert 1 galaxy NGC 5548 based on an analysis of all available archival data (from ROSAT, ASCA, Ginga, GRO/OSSE, and optical/IUE observations). We use this model as a framework to interpret correlated variability in the different bands, and thereby constrain the properties of the accretion flow.

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