The merging cluster Abell 1758: an optical and dynamical view (2015)
- Authors:
- USP affiliated authors: CYPRIANO, EDUARDO SERRA - IAG ; LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Assunto: AGLOMERADOS DE GALÁXIAS
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2015
- Source:
- Título do periódico: Meeting Abstracts
- Conference titles: IAU General Assembly
-
ABNT
MONTEIRO-OLIVEIRA, Rogério et al. The merging cluster Abell 1758: an optical and dynamical view. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 27 abr. 2024. -
APA
Monteiro-Oliveira, R., Cypriano, E. S., Machado, R., & Lima Neto, G. C. B. (2015). The merging cluster Abell 1758: an optical and dynamical view. In Meeting Abstracts. Paris: International Astronomical Union. -
NLM
Monteiro-Oliveira R, Cypriano ES, Machado R, Lima Neto GCB. The merging cluster Abell 1758: an optical and dynamical view. Meeting Abstracts. 2015 ;[citado 2024 abr. 27 ] -
Vancouver
Monteiro-Oliveira R, Cypriano ES, Machado R, Lima Neto GCB. The merging cluster Abell 1758: an optical and dynamical view. Meeting Abstracts. 2015 ;[citado 2024 abr. 27 ] - Mass profile and dynamical status of the z ∼ 0.8 galaxy cluster LCDCS 0504
- Simulating the shocks in the dissociative galaxy cluster Abell 1758N
- Weak lensing and spectroscopic analysis of the nearby dissociative merging galaxy cluster Abell 3376
- Investigating the merging cluster Abell 3376: weak lensing mass reconstruction
- Star formation efficiency in galaxy clusters
- Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4–0.9] redshift range
- Observations of a z=0.9 cluster of galaxies
- Cluster and cluster galaxy evolution history from IR to X-ray observations of the young cluster RX J1257.2+4738 at z=0.866
- A Gemini view of the galaxy cluster RXC J1504-0248: insights on the nature of the central gaseous filaments
- O aglomerado de galáxias RXC J1504-0248
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
