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Galactic Dynamos Without Sharp Boundaries: Non-Axisymmetric Fields in Axisymmetric Disks?

Published online by Cambridge University Press:  19 July 2016

R. Meinel
Affiliation:
Sternwarte Babelsberg Academy of Science Potsdam 1591 GDR
D. Elstner
Affiliation:
Sternwarte Babelsberg Academy of Science Potsdam 1591 GDR
G. Rüdiger
Affiliation:
Sternwarte Babelsberg Academy of Science Potsdam 1591 GDR
F. Krause
Affiliation:
Sternwarte Babelsberg Academy of Science Potsdam 1591 GDR

Extract

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Radio polarization observations of spiral galaxies suggest the existence of large-scale galactic magnetic fields which are of either axisymmetric -spiral (ASS) or bisymmetric-spiral (BSS), i.e. non-axisymmetric, structure (cf. Beck, 1939). Clear evidence for a BSS field was indicated for M31 by M. Krause et al. (1989).

Type
4. Magnetohydrodynamics of Galactic Magnetic Fields
Copyright
Copyright © Kluwer 1990 

References

Beck, R. (1989) ‘Present status of radio polarization observations’, Geophys. Astrophys. Fluid Dyn. (in press).Google Scholar
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Krause, M., Beck, R., and Hummel, E. (1989) ‘The magnetic field structure in two nearby spiral galaxies II. The bisymmetric spiral magnetic field in M81’, Astron. Astrophys. 217, 17.Google Scholar
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