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An overview of jet-mode AGN feedback and the prospects for studying its cosmic evolution with LOFAR

Published online by Cambridge University Press:  24 March 2015

L. Bîrzan ,
D. A. Rafferty ,
M. Brüggen  and
the LOFAR Team
L. Bîrzan
Affiliation:
Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029, Hamburg, Germany email: lbirzan@hs.uni-hamburg.de
D. A. Rafferty
Affiliation:
Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029, Hamburg, Germany email: lbirzan@hs.uni-hamburg.de
M. Brüggen
Affiliation:
Hamburger Sternwarte, Universität Hamburg, Gojenbergsweg 112, 21029, Hamburg, Germany email: lbirzan@hs.uni-hamburg.de
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Abstract

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Chandra revealed cavities in the hot atmospheres of many nearby clusters. These cavities are tracers of a strong coupling between the relativistic plasma in radio sources and the cooling, thermal gas in clusters. They demonstrate clearly that the AGN affects the cooling gas that leads to star formation and galaxy growth and allow a direct measurement of the bulk of the AGN's power. Together with radio data, the cavities allow us to derive scaling relations between mechanical (cavity) and radio power that can be used to estimate the AGN feedback power when direct measurement of the cavities is not possible. We review the importance of such relations for extending current studies of feedback with new and upcoming radio telescopes such as LOFAR and SKA.

Keywords

X-ray: galaxies: clusterscooling flowhigh redshiftradio continuum: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 251 - 259
Copyright
Copyright © International Astronomical Union 2015 

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