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Magnetic Fields of Radio Galaxies in Abell Clusters 115 and 568

Published online by Cambridge University Press:  19 July 2016

L. Gregorini ,
M. Bondi ,
L. Feretti ,
G. Giovannini  and
C.P. O'dea
L. Gregorini
Affiliation:
1 Dipartimento di Astronomia, Università di Bologna, Italy 2 Istituto di Radioastronomia del CNR, Bologna, Italy
M. Bondi
Affiliation:
2 Istituto di Radioastronomia del CNR, Bologna, Italy
L. Feretti
Affiliation:
1 Dipartimento di Astronomia, Università di Bologna, Italy 2 Istituto di Radioastronomia del CNR, Bologna, Italy
G. Giovannini
Affiliation:
1 Dipartimento di Astronomia, Università di Bologna, Italy 2 Istituto di Radioastronomia del CNR, Bologna, Italy
C.P. O'dea
Affiliation:
3 Netherland Foundation for Radio Astronomy, Dwingeloo, The Netherlands

Extract

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Abell 115 is an intermediate–redshift cluster (z=0.1971) well studied at different wavelengths (see Giovannini et al., 1987 and references therein).

Type
9. Magnetic Fields in the Galactic Environment, Galaxy Clusters and Intergalactic Medium
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 495 - 496
Copyright
Copyright © Kluwer 1990 

References

Giovannini, G., Feretti, L., Gregorini, L. (1987) Astron. Astrophys. Suppl. Ser. 69, 171 Google Scholar
Gregorini, L., Bondi, M. (1989) Astron. Astrophys. , in press Google Scholar