No CrossRef data available.
Article contents
Intracluster Magnetic Fields from X-ray and Radio Measurements
Published online by Cambridge University Press: 19 July 2016
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 combination of the observed diffuse radio and hard X-ray emission from clusters of galaxies is used to estimate lower limits on the intracluster magnetic field strength or upper limits on the energy density of the cosmic infrared background radiation.
- Type
- 9. Magnetic Fields in the Galactic Environment, Galaxy Clusters and Intergalactic Medium
- Information
- Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 487 - 491
- Copyright
- Copyright © Kluwer 1990
References
Bridle, A.H., Fomalont, E.B., Miley, G.K. and Valentijn, E.A. (1979) Astron. Astrophys.
80, 201.Google Scholar
Chandrasekhar, S. (1961) Hydrodynamic and Hydromagnetic Stability, Dover Publications, New York.Google Scholar
Roland, J., Sol, H., Pauliny–Toth, I. and Witzel, A. (1981) Astron. Astrophys.
100, 7.Google Scholar
You have
Access