Merging galaxy clusters produce low Mach number shocks in the intracluster medium. These shocks can accelerate electrons to relativistic energies that are detectable at radio frequencies
Radio relics are diffuse radio sources observed in galaxy clusters, probably produced by shock accel...
On the largest scales, the Universe consists of voids and filaments making up the cosmic web. Galaxy...
Galaxy clusters are the most massive constituents of the large-scale structure of the universe. Alth...
Merging galaxy clusters produce low Mach number shocks in the intracluster medium. These shocks can ...
The origin of radio relics is usually explained via diffusive shock acceleration (DSA) or re-acceler...
Diffuse radio emission in the form of radio haloes and relics has been found in a number of merging ...
Extended, steep, and ultra-steep spectrum radio emission in a galaxy cluster is usually associated w...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society:...
Previous studies have shown that CIZA J2242.8+5301 (the 'Sausage' cluster, z = 0.192) is a massive m...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We analysed a deep Chandra observation (334 ks) of the galaxy cluster Abell 115 and detected a shock...
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio g...
Diffuse synchrotron radio emission from cosmic ray electrons is observed at the centre of a number o...
LOFAR discovery of radio emission in MACSJ0717.5+3745 A. Bonafede, M. Brüggen, D. Rafferty, I. Zh...
The hot plasma within merging galaxy clusters is predicted to be filled with shocks and turbulence t...
Radio relics are diffuse radio sources observed in galaxy clusters, probably produced by shock accel...
On the largest scales, the Universe consists of voids and filaments making up the cosmic web. Galaxy...
Galaxy clusters are the most massive constituents of the large-scale structure of the universe. Alth...
Merging galaxy clusters produce low Mach number shocks in the intracluster medium. These shocks can ...
The origin of radio relics is usually explained via diffusive shock acceleration (DSA) or re-acceler...
Diffuse radio emission in the form of radio haloes and relics has been found in a number of merging ...
Extended, steep, and ultra-steep spectrum radio emission in a galaxy cluster is usually associated w...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society:...
Previous studies have shown that CIZA J2242.8+5301 (the 'Sausage' cluster, z = 0.192) is a massive m...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We analysed a deep Chandra observation (334 ks) of the galaxy cluster Abell 115 and detected a shock...
We report Chandra evidence for a 200 kpc scale shock in the cluster surrounding the powerful radio g...
Diffuse synchrotron radio emission from cosmic ray electrons is observed at the centre of a number o...
LOFAR discovery of radio emission in MACSJ0717.5+3745 A. Bonafede, M. Brüggen, D. Rafferty, I. Zh...
The hot plasma within merging galaxy clusters is predicted to be filled with shocks and turbulence t...
Radio relics are diffuse radio sources observed in galaxy clusters, probably produced by shock accel...
On the largest scales, the Universe consists of voids and filaments making up the cosmic web. Galaxy...
Galaxy clusters are the most massive constituents of the large-scale structure of the universe. Alth...