Spitzer observation of a 1763.: II. Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton Data (2010)
- Authors:
- Autor USP: LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Subjects: GALAXIAS; RAIOS X
- Language: Inglês
- Imprenta:
- Source:
- Título: The Astronomical Journal
- ISSN: 0004-6256
- Volume/Número/Paginação/Ano: v. 140, p. 1891-1904, 2010
-
ABNT
EDWARDS, Louise O. V et al. Spitzer observation of a 1763.: II. Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton Data. The Astronomical Journal, v. 140, p. 1891-1904, 2010Tradução . . Acesso em: 21 jan. 2026. -
APA
Edwards, L. O. V., Fadda, D., Frayer, D. T., Lima Neto, G. C. B., & Durret, F. (2010). Spitzer observation of a 1763.: II. Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton Data. The Astronomical Journal, 140, 1891-1904. -
NLM
Edwards LOV, Fadda D, Frayer DT, Lima Neto GCB, Durret F. Spitzer observation of a 1763.: II. Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton Data. The Astronomical Journal. 2010 ; 140 1891-1904.[citado 2026 jan. 21 ] -
Vancouver
Edwards LOV, Fadda D, Frayer DT, Lima Neto GCB, Durret F. Spitzer observation of a 1763.: II. Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton Data. The Astronomical Journal. 2010 ; 140 1891-1904.[citado 2026 jan. 21 ] - Some newly observed properties of elliptical galaxies
- An XMM-Newton view on relaxed and non-relaxed clusters of galaxies
- X-ray and optical substructures of the DAFT/FADA survey clusters
- Substructures in the intracluster gas
- The baryon fraction in five galaxy groups
- Giant ringlike radio structures around galaxy cluster Abell 3376
- Aglomerados de galáxias em altos redshifts
- A new method to quantify X-ray substructure in clusters of galaxies
- Spiral-like structure in the core of nearby galaxy clusters
- Efeitos da pressão de arraste em galáxias de aglomerados
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