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Unification of Radio Galaxies

Published online by Cambridge University Press:  12 April 2016

M.H. Cohen ,
P.M. Ogle ,
H.D. Iran  and
R.W. Goodrich
M.H. Cohen
Affiliation:
Caltech, Pasadena, CA 91125, U.S.A.
P.M. Ogle
Affiliation:
Caltech, Pasadena, CA 91125, U.S.A.
H.D. Iran
Affiliation:
IGPP, Lawrence Livermore National Laboratory, Livermore, CA 94550, U.S.A.
R.W. Goodrich
Affiliation:
W.M. Keck Observatory, Kamuela, HI 96743, U.S.A.

Abstract

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Many FR 2 narrow-line radio galaxies also display polarized broad lines. The broad-line region is hidden from direct view and is seen by reflection (ie scattering). In these objects the spectral classification is controlled by the aspect at which they are viewed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 81 - 82
Copyright
Copyright © Astronomical Society of the Pacific 1998

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