An important area of study of cosmic magnetic fields is on the largest scales, those of clusters of galaxies. In the last decade it has become clear that the intra-cluster medium in clusters of galaxies is magnetized and that magnetic fields play a critical role in the cluster formation and evolutio
Magnetic fields in halos of spiral galaxies
β Scribed by R.-J. Dettmar; M. Soida
- Publisher
- John Wiley and Sons
- Year
- 2006
- Tongue
- English
- Weight
- 529 KB
- Volume
- 327
- Category
- Article
- ISSN
- 0004-6337
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π SIMILAR VOLUMES
We present an exact solution for a static and axially symmetric spacetime, which is obtained from a scalar-tensor theory that comes from unification theories. As an attempt to model the dark matter (DM) in spiral galaxies we find that an exponential scalar potential is enough to explain the rotation
## Abstract We present here new images of relics and halo sources in rich cluster of galaxies and the correlation between the halo radio surface brightness versus the cluster bolometric Xβray luminosity. (Β© 2006 WILEYβVCH Verlag GmbH & Co. KGaA, Weinheim)