Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0751m&link_type=abstract
American Astronomical Society, HEAD meeting #9, #7.51; Bulletin of the American Astronomical Society, Vol. 38, p.358
Astronomy and Astrophysics
Astronomy
Scientific paper
AGN feedback plays a major role in models of galaxy formation, evolution, and black hole growth. However, observationally, the amount of feedback from AGN outflows is not well measured and most models assume an ad-hoc parameterization. We have, for the first time, measured accurately the outflow parameters in a Seyfert galaxy NGC 4051 using XMM data. We find that the mass loss in the outflow is only a few percent of the accretion rate and the outflow energy is only a small fraction of the radiative luminosity. If these physical characteristics are representative of AGN outflows, then they significantly fall short of the requirement for a susscessful feedback model. In this talk I will discuss our observational result and elaborate further on how feedback
Binette Luc
Brickhouse Nancy
Elvis Martin
Krongold Yair
Mathur Smita
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