Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-19T09:40:58.045Z Has data issue: false hasContentIssue false
  • English
  • Français

Jet-induced star formation: Good news from big, bad black holes

Published online by Cambridge University Press:  01 December 2004

Wil van Breugel ,
Chris Fragile ,
Stephen Croft ,
Wim de Vries ,
Peter Anninos  and
Stephen Murray
Wil van Breugel
Affiliation:
University of California, Lawrence Livermore National Laboratory, L-413, P.O. Box 808, Livermore, CA 94550, USA
Chris Fragile
Affiliation:
University of California, Lawrence Livermore National Laboratory, L-413, P.O. Box 808, Livermore, CA 94550, USA
Stephen Croft
Affiliation:
University of California, Lawrence Livermore National Laboratory, L-413, P.O. Box 808, Livermore, CA 94550, USA
Wim de Vries
Affiliation:
University of California, Lawrence Livermore National Laboratory, L-413, P.O. Box 808, Livermore, CA 94550, USA University of California at Davis, One Shields Ave, Davis, CA 95616, USA email: [email protected], [email protected], [email protected], [email protected], [email protected], [email protected]
Peter Anninos
Affiliation:
University of California, Lawrence Livermore National Laboratory, L-413, P.O. Box 808, Livermore, CA 94550, USA
Stephen Murray
Affiliation:
University of California, Lawrence Livermore National Laboratory, L-413, P.O. Box 808, Livermore, CA 94550, USA
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.

We discuss obbservations and numerical simulations which show that radiative shocks in jet-cloud collisions can trigger the collapse of intergalactic clouds and subsequent star formation in low luminosity, ‘FR-I’ type, radio galaxies.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
ORAL CONTRIBUTIONS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 485 - 488
Copyright
© 2004 International Astronomical Union