Westerbork observations at 610 MHz of the halo radio source in the Coma cluster are presented. It is shown that the total flux density of the radio source is 1.2 plus or minus 0.5 Jy and that its half-power Gaussian diameter is 33 arcmin. Furthermore it is argued that the highly polarized radio emission which was detected at the position of the Coma cluster is actually associated with an extended greater than 2 deg of arc Galactic feature. A lower limit of the intracluster magnetic-field strength of 1 ten-millionth G is derived
A 5 GHz study was carried out to study the fine-structure of five head-tail radio sources detected i...
In this thesis, we present 18 and 21 cm observations of the A773 galaxy cluster observed with the We...
Aims. Low-frequency radio observations of galaxy clusters are the key to detecting the diffuse exte...
Westerbork observations at 610 MHz of the halo radio source in the Coma cluster are presented. It is...
An area of 1.6 deg in radius about the centre of the Cancer Cluster has been surveyed at 610 MHz wit...
Abstract image available at: http://adsabs.harvard.edu/abs/1977A&AS...28..333
We present new measurements of the diffuse radio halo emission from the Coma cluster of galaxies at ...
We present new measurements of the diffuse radio halo emission from the Coma cluster of galaxies at ...
Abstract image available at: http://adsabs.harvard.edu/abs/1976A&A....49..179
Maps of the radio-brightness distribution at 5, 1.4, and 0.6 GHz of the wide-angle head-tail radio s...
Context. Radio halos and relics are diffuse radio sources found in galaxy clusters showing significa...
A map of the diffuse halo, Coma C, is constructed on the basis of observations of the Coma Cluster a...
Context. A fraction of galaxy clusters host diffuse radio sources called radio halos, radio relics a...
Context. The intra-cluster medium is characterized by thermal emission, and by the presence of larg...
Aims. To gain insight into the origin of diffuse radio sources in galaxy clusters and their connecti...
A 5 GHz study was carried out to study the fine-structure of five head-tail radio sources detected i...
In this thesis, we present 18 and 21 cm observations of the A773 galaxy cluster observed with the We...
Aims. Low-frequency radio observations of galaxy clusters are the key to detecting the diffuse exte...
Westerbork observations at 610 MHz of the halo radio source in the Coma cluster are presented. It is...
An area of 1.6 deg in radius about the centre of the Cancer Cluster has been surveyed at 610 MHz wit...
Abstract image available at: http://adsabs.harvard.edu/abs/1977A&AS...28..333
We present new measurements of the diffuse radio halo emission from the Coma cluster of galaxies at ...
We present new measurements of the diffuse radio halo emission from the Coma cluster of galaxies at ...
Abstract image available at: http://adsabs.harvard.edu/abs/1976A&A....49..179
Maps of the radio-brightness distribution at 5, 1.4, and 0.6 GHz of the wide-angle head-tail radio s...
Context. Radio halos and relics are diffuse radio sources found in galaxy clusters showing significa...
A map of the diffuse halo, Coma C, is constructed on the basis of observations of the Coma Cluster a...
Context. A fraction of galaxy clusters host diffuse radio sources called radio halos, radio relics a...
Context. The intra-cluster medium is characterized by thermal emission, and by the presence of larg...
Aims. To gain insight into the origin of diffuse radio sources in galaxy clusters and their connecti...
A 5 GHz study was carried out to study the fine-structure of five head-tail radio sources detected i...
In this thesis, we present 18 and 21 cm observations of the A773 galaxy cluster observed with the We...
Aims. Low-frequency radio observations of galaxy clusters are the key to detecting the diffuse exte...