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pro vyhledávání: '"Sikhosana, SP"'
Autor:
Venturi, T, Giacintucci, S, Merluzzi, P, Bardelli, S, Busarello, G, Dallacasa, D, Sikhosana, SP, Marvil, J, Smirnov, O, Bourdin, H, Mazzotta, P, Rossetti, M, Rudnick, L, Bernardi, G, Bruggen, M, Carretti, E, Cassano, R, Di Gennaro, G, Gastaldello, F, Kale, R, Knowles, K, Koribalski, BS, Heywood, I, Hopkins, AM, Norris, RP, Reiprich, TH, Tasse, C, Vernstrom, T, Zucca, E, Bester, LH, Diego, JM, Kanapathippillai, J
Publikováno v:
Astronomy & Astrophysics, 660:A81
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
et al.
[Context] The Shapley Supercluster (⟨z⟩≈0.048) contains several tens of gravitationally bound clusters and groups, making it an ideal subject for radio studies of cluster mergers.
[Aims] We used new high sensitivity radio obser
[Context] The Shapley Supercluster (⟨z⟩≈0.048) contains several tens of gravitationally bound clusters and groups, making it an ideal subject for radio studies of cluster mergers.
[Aims] We used new high sensitivity radio obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::700b7faea668b9970b061f728108328a
https://hdl.handle.net/2108/314372
https://hdl.handle.net/2108/314372
