A joint SZ–X-ray–optical analysis of the dynamical state of 288 massive galaxy clusters (2020)
- Authors:
- USP affiliated authors: LIMA, MARCOS VINICIUS BORGES TEIXEIRA - IF ; SILVA, MICHEL AGUENA DA - IF
- Unidade: IF
- DOI: 10.1093/mnras/staa1157
- Subjects: RAIOS X; GALÁXIAS
- Agências de fomento:
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- Volume/Número/Paginação/Ano: v. 495,n. 1, p. 705–725, 2020
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
ZENTENO, A e SILVA, Michel Aguena da e LIMA, Marcos Vinicius Borges Teixeira. A joint SZ–X-ray–optical analysis of the dynamical state of 288 massive galaxy clusters. Monthly Notices of the Royal Astronomical Society, v. 495, n. 1, p. 705–725, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa1157. Acesso em: 24 jan. 2026. -
APA
Zenteno, A., Silva, M. A. da, & Lima, M. V. B. T. (2020). A joint SZ–X-ray–optical analysis of the dynamical state of 288 massive galaxy clusters. Monthly Notices of the Royal Astronomical Society, 495( 1), 705–725. doi:10.1093/mnras/staa1157 -
NLM
Zenteno A, Silva MA da, Lima MVBT. A joint SZ–X-ray–optical analysis of the dynamical state of 288 massive galaxy clusters [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 495( 1): 705–725.[citado 2026 jan. 24 ] Available from: https://doi.org/10.1093/mnras/staa1157 -
Vancouver
Zenteno A, Silva MA da, Lima MVBT. A joint SZ–X-ray–optical analysis of the dynamical state of 288 massive galaxy clusters [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 495( 1): 705–725.[citado 2026 jan. 24 ] Available from: https://doi.org/10.1093/mnras/staa1157 - Candidate periodically variable quasars from the Dark Energy Survey and the Sloan Digital Sky Survey
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Informações sobre o DOI: 10.1093/mnras/staa1157 (Fonte: oaDOI API)
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