Hostname: page-component-7bb8b95d7b-pwrkn Total loading time: 0 Render date: 2024-09-27T03:05:03.805Z Has data issue: false hasContentIssue false
  • English
  • Français

Fast outflows of neutral hydrogen in radio galaxies

Published online by Cambridge University Press:  01 December 2004

T. A. Oosterloo ,
R. Morganti ,
B. H. C. Emonts  and
C. N. Tadhunter
T. A. Oosterloo
Affiliation:
Netherlands Foundation for Research in Astronomy, Postbus 2, NL-7990 AA, Dwingeloo, NL email: oosterloo@astron.nl
R. Morganti
Affiliation:
Netherlands Foundation for Research in Astronomy, Postbus 2, NL-7990 AA, Dwingeloo, NL email: oosterloo@astron.nl
B. H. C. Emonts
Affiliation:
Kapteyn Astronomical Institute, RuG, Landleven 12, 9747 AD, Groningen, NL
C. N. Tadhunter
Affiliation:
Dept. Physics & Astronomy, University of Sheffield, S7 3RH, UK
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

AGN activity is known to drive fast outflows of gas. We report the discovery of fast outflows of neutral gas with velocities over 1000 km/s in a number of radio galaxies. In the best studied object, 3C 293, the kinematical properties of the neutral and ionised outflows are similar, indicating a common origin. Moreover, the outflow appears to be located near the radio lobes and not near the nucleus. This suggests that the interaction between the radio jet and the ISM is driving the outflow.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 353 - 354
Copyright
© 2004 International Astronomical Union