A scaling relation between potential energy and mass for cluster elliptical galaxies (2000)
- Authors:
- Autor USP: LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Assunto: SISTEMA SOLAR
- Language: Inglês
- Imprenta:
- Source:
- Título: IAP 2000 meeting
- Conference titles: Conference on Construting the Universe with Clusters of Galaxies
-
ABNT
MÁRQUEZ, I et al. A scaling relation between potential energy and mass for cluster elliptical galaxies. 2000, Anais.. Paris: IAP, 2000. . Acesso em: 24 fev. 2026. -
APA
Márquez, I., Lima Neto, G. C. B., Capelato, H., Durret, F., Gerbal, D., & Lanzoni, B. (2000). A scaling relation between potential energy and mass for cluster elliptical galaxies. In IAP 2000 meeting. Paris: IAP. -
NLM
Márquez I, Lima Neto GCB, Capelato H, Durret F, Gerbal D, Lanzoni B. A scaling relation between potential energy and mass for cluster elliptical galaxies. IAP 2000 meeting. 2000 ;[citado 2026 fev. 24 ] -
Vancouver
Márquez I, Lima Neto GCB, Capelato H, Durret F, Gerbal D, Lanzoni B. A scaling relation between potential energy and mass for cluster elliptical galaxies. IAP 2000 meeting. 2000 ;[citado 2026 fev. 24 ] - Relaxed and unrelaxed clusters of galaxies seen in X-rays
- The merging cluster of galaxies Abell 3376: an optical view
- Spiral-like structure at the centre of nearby clusters of galaxies
- The merging cluster Abell 85 caught between meals by XMM-Newton
- A comprehensive picture of baryons in groups and clusters of galaxies
- An XMM-Newton view of the cluster of galaxies Abell 85
- Galaxy cluster as probes for cosmology and dark matter
- Perfil de temperatura e fração de bárions de aglomerados de galáxias em diferentes REDSHIFTS
- Physical properties of abell 85 intra-cluster medium
- Stellar formation in Brightest Cluster Galaxies
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