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Feedback in the Dark Domain

Published online by Cambridge University Press:  03 June 2010

Keiichi Wada
Keiichi Wada*
Affiliation:
National Astronomical Observatory of Japan Email: [email protected] Graduate School of Science and Engineering, Kagoshima University, Kagoshima 890-0065, Japan
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Abstract

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In order to clarify the physics of AGN feedback and feeding, we need to understand the interstellar medium (ISM) in the central several tens of parsecs in galaxies where our observational and theoretical knowledge is relatively poor. Here we discuss feedback processes due to strong far UV and X-ray radiation, as well as the dynamical effect of a supermassive black hole (SMBH) based on new high-resolution numerical simulations of the ISM in the central R ≤ 32 pc region around a SMBH at the center of a galaxy.

Keywords

methods: numericalgalaxies: evolutiongalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 362 - 369
Copyright
Copyright © International Astronomical Union 2010

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