A new method to quantify X-ray substructures in clusters of galaxies (2012)
Source: The Astrophysical Journal. Unidade: IAG
Subjects: GALÁXIAS, AGLOMERADOS DE GALÁXIAS, MEIO INTERGALÁTICO, ESTRUTURA DO UNIVERSO, RAIOS X
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ANDRADE-SANTOS, Felipe e LIMA NETO, Gastão César Bierrenbach e LAGANÁ, Tatiana Ferraz. A new method to quantify X-ray substructures in clusters of galaxies. The Astrophysical Journal, v. 746, p. 139/1-139/13, 2012Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/746/2/139. Acesso em: 15 out. 2024.APA
Andrade-Santos, F., Lima Neto, G. C. B., & Laganá, T. F. (2012). A new method to quantify X-ray substructures in clusters of galaxies. The Astrophysical Journal, 746, 139/1-139/13. doi:10.1088/0004-637X/746/2/139NLM
Andrade-Santos F, Lima Neto GCB, Laganá TF. A new method to quantify X-ray substructures in clusters of galaxies [Internet]. The Astrophysical Journal. 2012 ; 746 139/1-139/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/746/2/139Vancouver
Andrade-Santos F, Lima Neto GCB, Laganá TF. A new method to quantify X-ray substructures in clusters of galaxies [Internet]. The Astrophysical Journal. 2012 ; 746 139/1-139/13.[citado 2024 out. 15 ] Available from: https://doi.org/10.1088/0004-637X/746/2/139