An XMM-Newton view of the extended "filament" near the cluster of galaxies Abell 85 (2003)
- Authors:
- Autor USP: LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Assunto: MEIO INTERESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Astronomy and Astrophysics
- ISSN: 0004-6361
- Volume/Número/Paginação/Ano: v.403, p. L29-L32, 2003
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ABNT
DURRET, F et al. An XMM-Newton view of the extended "filament" near the cluster of galaxies Abell 85. Astronomy and Astrophysics, v. 403, p. L29-L32, 2003Tradução . . Acesso em: 12 mar. 2026. -
APA
Durret, F., Lima Neto, G. C. B., Forman, W., & Churazov, E. (2003). An XMM-Newton view of the extended "filament" near the cluster of galaxies Abell 85. Astronomy and Astrophysics, 403, L29-L32. -
NLM
Durret F, Lima Neto GCB, Forman W, Churazov E. An XMM-Newton view of the extended "filament" near the cluster of galaxies Abell 85. Astronomy and Astrophysics. 2003 ;403 L29-L32.[citado 2026 mar. 12 ] -
Vancouver
Durret F, Lima Neto GCB, Forman W, Churazov E. An XMM-Newton view of the extended "filament" near the cluster of galaxies Abell 85. Astronomy and Astrophysics. 2003 ;403 L29-L32.[citado 2026 mar. 12 ] - 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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