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/gamma 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
We conduct a multiwavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investi...
We analyze the results of long-term observations of the broad-line region (BLR) in the Seyfert 1 gal...
We derive power density spectra in the optical and X-ray band in the timescale range from several ye...
An extensive multi-satellite campaign on NGC 5548 has revealed this archetypal Seyfert-1 galaxy to b...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
We present our investigation into the long-term variability of the X-ray obscuration and optical-UV-...
International audienceWe present our investigation into the long-term variability of the X-ray obscu...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
An extensive multi-satellite campaign on NGC 5548 has revealed this archetypal Seyfert-1 galaxy to b...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
We present our investigation into the long-term variability of the X-ray obscuration and optical-UV-...
We model the spectral energy distribution of the type 1 Seyfert galaxy NGC 5548, fitting data from s...
An extensive multi-satellite campaign on NGC 5548 has revealed this archetypal Seyfert-1 galaxy to b...
We present the final installment of an intensive 13 year study of variations of the optical continuu...
We conduct a multiwavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investi...
We analyze the results of long-term observations of the broad-line region (BLR) in the Seyfert 1 gal...
We derive power density spectra in the optical and X-ray band in the timescale range from several ye...
An extensive multi-satellite campaign on NGC 5548 has revealed this archetypal Seyfert-1 galaxy to b...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
We present our investigation into the long-term variability of the X-ray obscuration and optical-UV-...
International audienceWe present our investigation into the long-term variability of the X-ray obscu...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
An extensive multi-satellite campaign on NGC 5548 has revealed this archetypal Seyfert-1 galaxy to b...
We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Tel...
We present our investigation into the long-term variability of the X-ray obscuration and optical-UV-...
We model the spectral energy distribution of the type 1 Seyfert galaxy NGC 5548, fitting data from s...
An extensive multi-satellite campaign on NGC 5548 has revealed this archetypal Seyfert-1 galaxy to b...
We present the final installment of an intensive 13 year study of variations of the optical continuu...
We conduct a multiwavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investi...
We analyze the results of long-term observations of the broad-line region (BLR) in the Seyfert 1 gal...
We derive power density spectra in the optical and X-ray band in the timescale range from several ye...