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Energy Transport in Radio Sources

Published online by Cambridge University Press:  30 March 2016

P. A. G. Scheuer
P. A. G. Scheuer*
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, England.

Extract

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Dr. Pacini has dealt with the innermost parsec; my job is to comment on the next 999,999. I have four comments.

1. A reminder of the importance of using the bulk kinetic energy of whatever beam or jet there is - forms of energy that exert pressure will get lost on the way out because of adiabatic expansion (Longair et al. 1973).

2. What is the asymmetry of jets trying to tell us?

Type
Joint Discussion
Information
Highlights of Astronomy , Volume 5: Highlights of Astronomy. As presented at the XVIIth General Assembly of the IAU, 1979 , 1980 , pp. 667 - 669
Copyright
Copyright © Cambridge University Press 1980

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