𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Magnetic fields in clusters of galaxies

✍ Scribed by L. Feretti; M. Johnston-Hollitt


Publisher
Elsevier Science
Year
2004
Tongue
English
Weight
358 KB
Volume
48
Category
Article
ISSN
1387-6473

No coin nor oath required. For personal study only.

✦ Synopsis


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 evolution. The observational evidence for the existence of cluster magnetic fields is obtained by the diffuse cluster-wide synchrotron radio emission and from rotation measure studies of extragalactic radio sources located within or behind the clusters. A significant breakthrough in the knowledge of the cluster magnetic fields will be reached through the SKA, owing to its capabilities, in particular the deep sensitivity and the polarization purity.


πŸ“œ SIMILAR VOLUMES


Fast growth of magnetic fields in galaxy
✍ A. A. Schekochihin; S. C. Cowley πŸ“‚ Article πŸ“… 2006 πŸ› John Wiley and Sons 🌐 English βš– 155 KB πŸ‘ 2 views

## Abstract We propose a model of magnetic‐field growth in galaxy clusters whereby the field is ampli.fied by a factor of about 10^8^ over a cosmologically short time of ∼ 10^8^ yr. Our model is based on the idea that the viscosity of the intracluster medium during the field‐amplification epoch is

Magnetic turbulence in cool cores of gal
✍ C. Vogt; T. A. Enßlin πŸ“‚ Article πŸ“… 2006 πŸ› John Wiley and Sons 🌐 English βš– 102 KB πŸ‘ 2 views

## Abstract The analysis of Faraday rotation measurements (RM) gives insight into the properties of cluster magnetic fields. Recently, Kolmogorov‐like magnetic turbulence was reported for the cool core of the Hydra A galaxy cluster which was derived using a maximum likelihood analysis of an RM map