The Coma cluster at LOFAR frequencies. II. The halo, relic, and a new accretion relic

Author(s):
Bonafede, A.; Brunetti, G.; Rudnick, L.; Vazza, F.; Bourdin, H.; Giovannini, G.; Shimwell, T.W.; Zhang, X. (0000-0001-6019-6373); Mazzotta, P.; Simionescu, A.; Biava, N.; Bonnassieux, E.; Brienza, M.; Brüggen, M.; Rajpurohit, K.; Riseley, C.J.; Stuardi, C.; Feretti, L.; Tasse, C.; Botteon, A. (0000-0002-9325-1567); Carretti, E.; Cassano, R.; Cuciti, V.; Gasperin, F. de .; Gastaldello, F.; Rossetti, M.; Rottgering, H.J.A. (0000-0001-8887-2257); Venturi, T.; Weeren, R.J. van .
Published
2022
Publication type
Article / Letter to editor
Galaxy clustersNon-thermal radiation sourcesExtragalactic radio sourcesIntracluster medium5841119508858Astrophysics - high energy astrophysical phenomenaAstrophysics - cosmology and nongalactic astrophysics
Date issued
2022
Language
English
Is part of
The Astrophysical Journal (2022), No. 2, 218
hdl
1887/3561358
doi
10.3847/1538-4357/ac721d
URL
https://ui.adsabs.harvard.edu/abs/2022ApJ...933..218B