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Magnetic Fields and Star Formation for the ANS Sample of Galaxies

Published online by Cambridge University Press:  19 July 2016

J. Stryczynski
J. Stryczynski*
Affiliation:
Torun Radio Astronomy Observatory N. Copernicus University ul. Chopin a 12/18 87-100 Torun, Poland

Abstract

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From the literature we collected radio and magnetic field data for the ANS spiral galaxies. We suggest that the groups of objects, as revealed in the UV range, do not differ in magnetic field strength, although statistics of the sample are very poor.

Type
5. The Polarization, Magnetic Field and Velocity Structure of External Spiral Galaxies
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 233 - 234
Copyright
Copyright © Kluwer 1990 

References

Duric, N., Bourneuf, E. and Gregory, P.C. (1988) Astron. J. 96, 81.Google Scholar
Klein, U. (1988) Radio Emission and Star Formation in Spiral and Dwarf Irregular Galaxies , Habilitationsschrift Universität Bonn Google Scholar
Moffet, A.T. (1975) in Sandage, A., Sandage, M. and Kristian, J. (eds.), Galaxies in the Universe, Volume IX of Stars and Stellar Systems, The University of Chicago Press, p. 211.Google Scholar
Stryczynski, J. (1987) Astron. Astrophys. Suppl. 70, 115.Google Scholar
Wesselius, P.R., van Duinen, R.J., de Jonge, A.R.W., Aalders, J.W.G., Luinge, W. and Wildeman, K.J. (1982) Astron. Astrophys. Suppl. 49, 427.Google Scholar
Wunderlich, E. and Klein, U. (1988) Astron. Astrophys. 206, 47.Google Scholar