Hostname: page-component-76fb5796d-skm99 Total loading time: 0 Render date: 2024-04-27T21:53:34.291Z Has data issue: false hasContentIssue false
  • English
  • Français

A Self-Similar Model for Extragalactic Jets and the FRI/FRII Divide

Published online by Cambridge University Press:  12 April 2016

C.R. Kaiser  and
P. Alexander
C.R. Kaiser
Affiliation:
MRAO, Cavendish Lab., Madingley Road, Cambridge, CBS OHE, UK
P. Alexander
Affiliation:
MRAO, Cavendish Lab., Madingley Road, Cambridge, CBS OHE, UK

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 present a model for the large scale structure of FRIItype extragalactic radio sources. The sources are shown to grow selfsimilar and the dependence of the length of the source and the pressure inside the cocoon on the life time are calculated. The stability of the jets in such sources is investigated and the jet power at which FRII sources turn into FRIs is found to be in good agreement with observations.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 732 - 733
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Cantó, J., and Raga, A.C. 1991, ApJ, 372, 646 Google Scholar
Falle, S.A.E.G. 1991, MNRAS, 250, 581 CrossRefGoogle Scholar
Rawlings, S., and Saunders, R. 1991, Nature, 349, 138 Google Scholar
Scheuer, P.A.G. 1974, MNRAS, 166, 513 Google Scholar