Mass Outflows from Seyfert Galaxies as Seen in Emission and Absorption

Details Mass Outflows from Seyfert Galaxies as Seen in Emission and Absorption Mass Outflows from Seyfert Galaxies as Seen in Emission and Absorption

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..319c&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Physics

Scientific paper

We summarize the observational properties of the outflowing UV/X-ray absorbers in Seyfert galaxies and the constraints that they impose on dynamical models, including accretion-disk winds. We examine recent evidence that the absorbers have been detected in emission, and discuss the implications of these results for determining the nature of the mass outflows.

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