Determining AGN Feedback Parameters from Seyfert Galaxy Outflows

Details Determining AGN Feedback Parameters from Seyfert Galaxy Outflows Determining AGN Feedback Parameters from Seyfert Galaxy Outflows

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21714214c&link_type=abstract

American Astronomical Society, AAS Meeting #217, #142.14; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Mass outflows of ionized gas, detected through Hubble Space Telescope observations of blueshifted UV absorption lines and spatially-resolved emission lines, are common in nearby AGN. We review the constraints that these observations place on the structure of AGN winds, and provide estimates of the mass outflow rates and kinematic luminosities needed for AGN feedback models.

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