No CrossRef data available.
Article contents
Radio Studies of Cosmic Rays in Nearby Galaxies
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.
The constraints on cosmic ray electron sources and propagation as derived from radio continuum observations of galaxies are reviewed. Special attention is paid to the inferences which can be obtained from the radio continuum properties of spiral galaxies seen edge-on.
- Type
- II. The Disk-Halo Interface in Other Galaxies
- Information
- Copyright
- Copyright © Kluwer 1991
References
REFERENCES
Allen, R.J., Hu, F.X.: 1985, in
New Aspects of Galaxy Photometry
ed. Nieto, J.L., p293
CrossRefGoogle Scholar
Hummel, E.: 1990, in
Windows on Galaxies
, eds. Fabbiano, G., Gallagher, J.S. and Renzini, A., Kluwer, Dordrecht, p141
Google Scholar
Hummel, E., Davies, R.D., Wolstencroft, R.D., van der Hulst, J.M., Pedlar, A.: 1988,
Astron. Astrophys.
, 199, 91
Google Scholar
Hummel, E., Dahlem, M., van der Hulst, J.M., Sukumar, S.: 1990,
Astron. Astrophys.
, in press
Google Scholar
Klein, U.: 1990, in
Windows on Galaxies
, eds. Fabbiano, G., Gallagher, J.S. and Renzini, A., Kluwer, Dordrecht, p157
CrossRefGoogle Scholar
Krause, M.: 1990, in
Galactic and Intergalactic Magnetic Fields
, eds. Beck, R., Kronberg, P.P. and Wielebinski, R., Kluwer, Dordrecht, p187
Google Scholar