No CrossRef data available.
Article contents
Magnetic Fields in the Disk-Halo Interface
Published online by Cambridge University Press: 03 August 2017
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
A review is given of large-scale magnetic fields in disks and halos of spiral galaxies. A particular attention is given to vertical field structures, and we discuss their origin and implication on their interaction with halo gas. We point out that the disk-halo magnetic interface plays an important role in circulation of interstellar gas in galaxies, in particular a large-scale circulartion from the galactic center to outer disk regions.
- Type
- I. The Disk-Halo Interface in Our Galaxy
- Information
- Copyright
- Copyright © Kluwer 1991
References
REFERENCES
Berkhuijsen, E.M., Beck, R., and Gräve, R.
1987, in
Interstellar Magnetic Fields
, ed. Beck, R. and Gräve, R. (Springer Verlag, Berlin), p.38.Google Scholar
Hummel, E., Lesch, H., Wielebinski, R., Schilickerser, R.
1988,
Astron. Astrophys. Letters
, 197, L29.Google Scholar
Sofue, Y., Fujimoto, M., and Wielebinski, R.
1986,
Ann. Rev. Astron. Astrophys.
, 24, 459.Google Scholar
Sofue, Y., Reich, W., Inoue, M., and Seiradakis, J.H.
1987,
Publ. Astron. Soc. Japan
, 39, 359.Google Scholar
Tsuboi, M., Inoue, M., Handa, T., Tabara, H., Kato, T., Sofue, Y., and Kaifu, N.
1986,
Astron. J.
, 92, 818.Google Scholar