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The magnetic-field structure and dynamics of NGC 253

Published online by Cambridge University Press:  04 August 2017

M. Urbanik
Affiliation:
Astronomical Observatory Jagiellonian University, Krakow, Poland
U. Klein
Affiliation:
Max-Planck-Institut für Radioastronomie Bonn, West-Germany
R. Beck
Affiliation:
Max-Planck-Institut für Radioastronomie Bonn, West-Germany
R. Wielebinski
Affiliation:
Max-Planck-Institut für Radioastronomie Bonn, West-Germany

Abstract

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Total-power and polarization observations of NGC 253 at 10.7 GHz have been performed with the 100-m MPIfR radio telescope. The observed arm/interarm polarization contrasts are discussed in the context of possible field configurations in spiral arms.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Copyright
Copyright © Reidel 1985 

References

Elmegreen, B.G., 1982, Astrophys. J. 253, p. 655.Google Scholar
Mouschovias, T.C., Shu, F.H., Woodward, P.R., 1974, Astron. Astrophys. 33, p. 73.Google Scholar
Parker, E.N., 1966, Astrophys. J. 145, p. 811.Google Scholar
Soukup, J.E., Yuan, C., 1981, Astrophys. J. 246, p. 376.Google Scholar
Tubbs, A.D., 1980, Astrophys. J. 239, p. 882.Google Scholar