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Global Magnetic Structure In Spiral Galaxies

Published online by Cambridge University Press:  25 April 2016

S. J. Spencer
S. J. Spencer*
Affiliation:
School of Physics, University of Sydney, 2006 NSW
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Abstract

Global magnetic structure has been inferred in spiral galaxies from radio and optical observations. The author has developed a three dimensional, quasi-global kinematic dynamo model which demonstrates the possibility of maintaining large-scale magnetic fields by the αω mechanism. Analytical expressions for large-scale galactic magnetic fields near temporal steady states have been derived. Illustrations of the spatial distribution of vector and absolute large-scale magnetic field strength are presented. When coupled with observations this model may help in understanding the maintenance and morphologies inferred for disk and halo global magnetic fields in spiral galaxies.

Type
Extragalactic
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 1 , 1991 , pp. 95 - 97
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Asseo, E. and Sol, H., 1987, Physics Reports, 148, 307.CrossRefGoogle Scholar
Beck, R., 1982, Astron. Astrophys., 106, 121.Google Scholar
Fujimoto, M. and Sawa, T., 1987, Publ. Astron. Soc. Japan, 39, 375.Google Scholar
Krause, F. and Radler, K. H., 1980, Mean Field Magnetohydrodynamics and Dynamo Theory, Akademie Verlag, Berlin.Google Scholar
Krause, M., Beck, R. and Hummel, E., 1987, Proc. Int. Mag. Fields Obs. and Theory, eds. Beck, R. and Grave, R., p. 57.Google Scholar
Krause, M., Hummel, E. and Beck, R., 1988, MPIFR Preprint Series, No. 341.Google Scholar
Layzer, D., Rosner, R. and Doyle, H. T., 1979, Astrophys. J., 229, 1126.CrossRefGoogle Scholar
Lesen, H. et al., 1989, MPIFR Preprint Series, No. 344.Google Scholar
Moffatt, H. K., 1983, Stellar and Planetary Magnetism, 3, ed. Soward, A. M..Google Scholar
Parker, E. N., 1970, Astroplvys. J., 162, 665.CrossRefGoogle Scholar
Parker, E. N., 1971a, Astrophys. J., 163, 255.Google Scholar
Parker, E. N., 1971b, Astrophys. J., 163, 279.Google Scholar
Parker, E. N., 1979, Cosmical Magnetic Fields, Clarendon Press, Oxford.Google Scholar
Radler, K. H., 1983a, Stellar and Planetary Magnetism, 17, ed. Soward, A. M..Google Scholar
Radler, K. H., 1983b, Stellar and Planetary Magnetism, 37, ed. Soward, A. M..Google Scholar
Ruzmaikin, A. A., Shukurov, A. M. and Sokoloff, D. D., 1988, Magnetic Fields of Galaxies, Kluwer Academic, London.Google Scholar
Sawa, T. and Fujimoto, M., 1986, Publ. Astron. Soc. Japan, 38, 133.Google Scholar
Sofue, Y., Klein, U.. Beck, R. and Wielebinski, R., 1985, Astron. Astrophys., 144, 257.Google Scholar
Sofue, Y., Fujimoto, M.and Wielebinski, R., 1986, Annu. Rev. Astron. Astrophys., 24, 459.Google Scholar