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Gas Outflows in Radio Galaxies

Published online by Cambridge University Press:  26 May 2016

R. Morganti ,
T. Oosterloo ,
B.H.C. Emonts ,
C. N. Tadhunter  and
J. Holt
R. Morganti
Affiliation:
Netherlands Foundation for Research in Astronomy, Postbus 2, NL-7990 AA, Dwingeloo, The Netherlands
T. Oosterloo
Affiliation:
Netherlands Foundation for Research in Astronomy, Postbus 2, NL-7990 AA, Dwingeloo, The Netherlands
B.H.C. Emonts
Affiliation:
Kapteyn Astronomical Institute, RuG, Landleven 12, 9747 AD, Groningen, The Netherlands
C. N. Tadhunter
Affiliation:
Dept. Physics & Astronomy, University of Sheffield, S7 3RH, UK
J. Holt
Affiliation:
Dept. Physics & Astronomy, University of Sheffield, S7 3RH, UK

Abstract

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We present a summary of our recent results on gas outflows in radio galaxies. Fast outflows (up to 2000 km s−1) have been detected both in ionized and neutral gas. The latter is particularly surprising as it shows that, despite the extremely energetic phenomena occurring near an AGN, some of the outflowing gas remains, or becomes again, neutral. These results are giving new and important insights on the physical conditions of the gaseous medium around an AGN.

Type
Part 3. Ejection and Outflow
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 332 - 337
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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