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11.18. The magnetic switch and the FR I/FR II break

Published online by Cambridge University Press:  25 May 2016

D.L. Meier ,
P. Godon ,
S. Edgington ,
D.G. Payne  and
K.R. Lind
D.L. Meier
Affiliation:
Jet Propulsion Laboratory, Caltech, Pasadena, CA, USA
P. Godon
Affiliation:
Jet Propulsion Laboratory, Caltech, Pasadena, CA, USA
S. Edgington
Affiliation:
Jet Propulsion Laboratory, Caltech, Pasadena, CA, USA
D.G. Payne
Affiliation:
Jet Propulsion Laboratory, Caltech, Pasadena, CA, USA
K.R. Lind
Affiliation:
Digital Equipment Corporation, Livermore, CA, USA

Abstract

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It is proposed that the Fanaroff and Riley division between class I and class II radio sources may be due to phenomena occurring in the coronae of magnetized accretion disks around black holes.

Type
Part III. Black Holes and Central Activity
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 491 - 492
Copyright
Copyright © Kluwer 1998 

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