Evidence for particle re-acceleration in the radio relic in the galaxy cluster PLCKG287.0+32.9
Radio relics are diffuse radio sources observed in galaxy clusters, probably produced by shock acceleration during cluster-cluster mergers. Their large size, of the order of 1 Mpc, indicates that the emitting electrons need to be (re)accelerated locally. The usually invoked diffusive shock accelerat...
| Main Authors: | Bonafede, A., Intema, Hubertus, Brüggen, M., Girardi, M., Nonino, M., Kantharia, N., Van Weeren, R., Röttgering, H. |
|---|---|
| Format: | Journal Article |
| Published: |
Institute of Physics Publishing
2014
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| Online Access: | http://hdl.handle.net/20.500.11937/74569 |
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