Cover Page The handle

It is proposed that these radio relics trace shock waves in the intracluster medium (ICM) created during a cluster merger event.. Within the shock waves particles are accelerated

Here we report the detection of a radio relic for which we find highly aligned magnetic fields, a strong spectral index gradient, and a narrow relic width, giving a measure of

In this section we present the simulated radio maps for a range of mass ratios, impact parame- ters, viewing angles and radial density/temperature profiles, and compare them to

The LOFAR 63 MHz image reveals some of the well-known tailed radio sources (A, B, F), the main relic (G and H), and part of the radio halo.. A hint of the long and straight

2004, in Presented at the Society of Photo- Optical Instrumentation Engineers (SPIE) Conference, Vol.. 5489, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference

Door deze gegevens te combineren met al bekende radio relics zijn correlaties gevonden tussen verschillende eigenschappen van de bronnen, zoals hun grootte en de mate waarin

Tijdens de doctoraalfase van mijn studie heb ik gewerkt aan radio waarnemingen van de cluster van sterrenstelsels Abell 2256, onder leiding van Prof.. Deze waarnemingen waren gedaan

The compilation of large unbiased samples of radio relics and halos will be crucial for our understanding of shocks, turbulence, particle acceleration and magnetic fields in