In a growing number of galaxy clusters diffuse extended radio sources have been found.
These sources are not directly associated with individual cluster galaxies. The radio …

Clusters of galaxies are gravitationally bound configurations containing typically hundreds of
galaxies in a region about 10 25 cm in size. They range from irregular clusters, with strong …

We present evidence for the existence of shock waves caused by the formation of the large-
scale structure. In some clusters of galaxies peripherally located sources of extended diffuse …

Detection of excess rotation measure due to intracluster magnetic fields in clus ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

We present in this paper the first high-resolution spectral index map of the halo source
Coma C, which was obtained combining WSRT data at 326 MHz and DRAO+ VLA data at …

The halo and magnetic field of the Coma cluster of galaxies ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …

We present a numerical model for the extended steep-spectrum radio sources and the
elongated X-ray structure in A3667 based on new three-dimensional MHD/N-body …

We present new measurements of the diffuse radio halo emission from the Coma cluster of
galaxies at 2.675 GHz and 4.85 GHz using the Effelsberg 100–m telescope. After correction …

New measurements of the diffuse radio halo from the Coma cluster at a wavelength λ11 cm
are presented. After correcting for the contribution from point sources the authors derived the …

THE Coma cluster is a rich cluster of galaxies nested in an even larger supercluster of
galaxies. The plane of the supercluster seems to be defined by the Coma cluster itself and …