Abstract
Interstellar magnetic fields are known to be a constraint for star formation, but their influence on the formation of spiral structures and the evolution of galaxies is generally neglected. Structure, strength and degree of uniformity of interstellar magnetic fields can be determined by measuring the linearly polarised radio continuum emission at several frequencies (e.g. Beck, 1982). Results for 7 galaxies observed until now with the Effelsberg and Westerbork radio telescopes are given in the table. The Milky Way is also included for comparison.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
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1. Magnetic Fields of Galaxies;Interstellar Magnetic Fields;1987
2. Nonthermal Radio Emission from the Galaxy;Galactic Astrophysics and Gamma-Ray Astronomy;1983