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Galactic Winds and Magnetic Fields from Spiral Galaxies

Published online by Cambridge University Press:  19 July 2016

H.J. Völk ,
D. Breitschwerdt  and
J.F. McKenzie
H.J. Völk
Affiliation:
1Max-Planck-Institut für Kernphysik, Heidelberg
D. Breitschwerdt
Affiliation:
1Max-Planck-Institut für Kernphysik, Heidelberg
J.F. McKenzie
Affiliation:
2Max-Planck-Institut für Aeronomie, Lindau

Extract

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Concentrating on our own Galaxy we discuss the dynamics of the outer halo, its magnetic structure and the occurrence of a supersonic mass loss in the form of a Galactic wind. The cosmic rays, as the nonthermal high energy component, de facto not influenced by gravity, play an essential role in the wind dynamics.

Type
4. Magnetohydrodynamics of Galactic Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 177 - 181
Copyright
Copyright © Kluwer 1990 

References

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