A LOFAR study of non-merging massive galaxy clusters

A LOFAR study of non-merging massive galaxy clusters

Centrally located diffuse radio emission has been observed in both merging and non-merging galaxy clusters. Depending on their morphology and size, we distinguish between giant radio haloes, which occur predominantly in merging clusters, and mini haloes, which are found in non-merging, cool-core clu...

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Bibliographic Details
Main Authors: Savini, F., Bonafede, A., Brüggen, M., Rafferty, D., Shimwell, T., Botteon, A., Brunetti, G., Intema, Huib, Wilber, A., Cassano, R., Vazza, F., Van Weeren, R., Cuciti, V., De Gasperin, F., Röttgering, H., Sommer, M., Bîrzan, L., Drabent, A.
Format: Journal Article
Language:English
Published: EDP SCIENCES S A 2019
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
techniques: interferometric
acceleration of particles
surveys
galaxies: clusters: general
galaxies: clusters: intracluster medium
radio continuum: general
DIFFUSE RADIO-EMISSION
COOL-CORE CLUSTERS
COSMIC-RAYS
GAMMA-RAY
HALOS
STATISTICS
SEARCH
ORIGIN
PLASMA
IMAGES
Online Access:http://hdl.handle.net/20.500.11937/76019

Internet

http://hdl.handle.net/20.500.11937/76019

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