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Comparison of Radio and Optical Polarization in Extended Extragalactic Radio Sources: II. Implications for the Magnetic Fields

Published online by Cambridge University Press:  19 July 2016

K. Meisenheimer  and
H.-J. Röser
K. Meisenheimer
Affiliation:
Max-Planck-Institut für Astronomie Königsiuhl 17, D-6900 Heidelberg 1 Federal Republic of Germany
H.-J. Röser
Affiliation:
Max-Planck-Institut für Astronomie Königsiuhl 17, D-6900 Heidelberg 1 Federal Republic of Germany

Extract

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Although optical synchrotron light from an extragalactic source - the jet in M 87 - has been discovered more than 30 years ago (Baade 1956) there are still only a handful extended radio sources with established optical synchrotron emission (see Röser 1989 and references therein, also Meisenheimer et al. 1989b). We outline the relevance of optical studies and summarize some results concerning the magnetic fields in extragalactic radio sources.

Type
8. The Role of Magnetic Fields in Radio Source Jets and Extended Radio Lobes
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 451 - 452
Copyright
Copyright © Kluwer 1990 

References

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