Dusty and distant galaxies inside and out an X-ray luminous cluster (2011)
- Authors:
- Autor USP: LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Subjects: GALÁXIAS; RAIOS X
- Language: Inglês
- Imprenta:
- Publisher: XMM-Newton Science Operations Centre
- Publisher place: Paris
- Date published: 2011
- Source:
- Conference titles: Conference on the X-Ray Universe 2011
-
ABNT
ULMER, Melville et al. Dusty and distant galaxies inside and out an X-ray luminous cluster. 2011, Anais.. Paris: XMM-Newton Science Operations Centre, 2011. . Acesso em: 10 jan. 2026. -
APA
Ulmer, M., Adami, C., Durret, F., Lima Neto, G. C. B., Chary, R. -R., Davies, J., & Guennou, L. (2011). Dusty and distant galaxies inside and out an X-ray luminous cluster. In Abstract book: oral communications and posters. Paris: XMM-Newton Science Operations Centre. -
NLM
Ulmer M, Adami C, Durret F, Lima Neto GCB, Chary R-R, Davies J, Guennou L. Dusty and distant galaxies inside and out an X-ray luminous cluster. Abstract book: oral communications and posters. 2011 ;[citado 2026 jan. 10 ] -
Vancouver
Ulmer M, Adami C, Durret F, Lima Neto GCB, Chary R-R, Davies J, Guennou L. Dusty and distant galaxies inside and out an X-ray luminous cluster. Abstract book: oral communications and posters. 2011 ;[citado 2026 jan. 10 ] - X-ray and optical substructures of the DAFT/FADA survey clusters
- An XMM-Newton view on relaxed and non-relaxed clusters of galaxies
- Cl 1205+44: afossil group at'IND z'=0.59
- A new method to quantify X-ray substructure in clusters of galaxies
- Spiral-like structure in the core of nearby galaxy clusters
- Galaxy clusters seen in X-rays: from the most relaxed to the most perturbed
- Efeitos da pressão de arraste em galáxias de aglomerados
- Quantifying X-ray substructures in clusters of galaxies
- Cosmologia
- Correlações baseadas na entropia específica de galáxias elípticas
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