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Evidence of a Large Scale Magnetic Field in the Coma - A1367 Supercluster

Published online by Cambridge University Press:  19 July 2016

G. Giovannini ,
K.-T. Kim ,
P. P. Kronberg  and
T. Venturi
G. Giovannini
Affiliation:
(1) Dipartimento di Astronomia, via Zamboni 33, I-40100 Bologna ITALY (2) Istituto di Radioastronomia, via Irnerio 46, I-40126 Bologna, ITALY
K.-T. Kim
Affiliation:
(3) Department of Astronomy, University of Toronto, Toronto Ontario M5S 1A7, CANADA
P. P. Kronberg
Affiliation:
(3) Department of Astronomy, University of Toronto, Toronto Ontario M5S 1A7, CANADA
T. Venturi
Affiliation:
(2) Istituto di Radioastronomia, via Irnerio 46, I-40126 Bologna, ITALY

Extract

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The Coma cluster is a rich cluster of galaxies nested in an even larger supercluster of galaxies. The plane of the supercluster appears to be defined by the Coma cluster itself and another galaxy cluster, Abell 1367, that lies about 40 Mpc (H0 = 75 Mpc km−1s−1 (≡h75)) farther west (Tifft and Gregory 1976).

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. 492 - 494
Copyright
Copyright © Kluwer 1990 

References

Andernach, H., Feretti, L., Giovannini, G. 1984, Astron. Astrophys. , 133, 242.Google Scholar
Tifft, W. G., and Gregory, S. A. 1976, Ap. J. , 205, 696.CrossRefGoogle Scholar
Willson, M. A. G. 1970, Mon. Not. R. Astron. Soc. , 151, 1.CrossRefGoogle Scholar