Radio observations of the merging galaxy cluster Abell 520

Radio observations of the merging galaxy cluster Abell 520

Context. Extended synchrotron radio sources are often observed in merging galaxy clusters. Studies of the extended emission help us to understand the mechanisms in which the radio emitting particles gain their relativistic energies. Aims. We examine the possible acceleration mechanisms of the relati...

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Bibliographic Details
Main Authors: Hoang, D.N., Shimwell, T.W., Van Weeren, R.J., Brunetti, G., Röttgering, H.J.A., Andrade-Santos, F., Botteon, A., Brüggen, M., Cassano, R., Drabent, A., De Gasperin, F., Hoeft, M., Intema, Huib, Rafferty, D.A., Shweta, A., Stroe, A.
Format: Journal Article
Language:English
Published: EDP SCIENCES S A 2019
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
acceleration of particles
galaxies: clusters: individual: Abell 520
galaxies: clusters: intracluster medium
large-scale structure of Universe
PARTICLE-ACCELERATION
COSMIC-RAYS
SCALING RELATIONS
MAGNETIC-FIELDS
BULLET CLUSTER
LOW-FREQUENCY
SHOCK FRONTS
COLD FRONTS
TURBULENCE
ORIGIN
Online Access:http://hdl.handle.net/20.500.11937/76027

Internet

http://hdl.handle.net/20.500.11937/76027

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