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AGN feedback from jet-ISM/IGM interactions

Published online by Cambridge University Press:  01 July 2007

V. Antonuccio-Delogu  and
J. Silk
V. Antonuccio-Delogu
Affiliation:
Department of Physics, University of Oxford, Keble Road, OX1 3RH, Oxford, United Kingdom email: van@astro.ox.ac.uk, silk@astro.ox.ac.uk INAF, Osservatorio Astrofisico di Catania, Via S. Sofia 78, I-95123 Catania, Italy
J. Silk
Affiliation:
Department of Physics, University of Oxford, Keble Road, OX1 3RH, Oxford, United Kingdom email: van@astro.ox.ac.uk, silk@astro.ox.ac.uk
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Abstract

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We study the propagation of relativistic jets originating from AGNs within the Interstellar/Intergalactic Medium of their host galaxies, and use it to build a model for the inihibition of stellar formation within the expanding cocoon.

Keywords

galaxies: jetsgalaxies: bulgesgalaxies: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 31 - 32
Copyright
Copyright © International Astronomical Union 2008

References

Falle, S. A. E. G. 1991, MNRAS 250, 581CrossRefGoogle Scholar
Kaiser, C. R. & Alexander, P. 1997, MNRAS 286, 215CrossRefGoogle Scholar