The galaxy cluster RXC J1504-0248: a remarkable cool core near us (2015)
- Authors:
- USP affiliated authors: SODRE JUNIOR, LAERTE - IAG ; CYPRIANO, EDUARDO SERRA - IAG ; LIMA NETO, GASTAO CESAR BIERRENBACH - IAG
- Unidade: IAG
- Subjects: AGLOMERADOS DE GALÁXIAS; FORMAÇÃO DE ESTRELAS
- Language: Inglês
- Imprenta:
- Publisher: International Astronomical Union
- Publisher place: Paris
- Date published: 2015
- Source:
- Título: Meeting Abstracts
- Conference titles: IAU General Assembly
-
ABNT
SOJA, A. C et al. The galaxy cluster RXC J1504-0248: a remarkable cool core near us. 2015, Anais.. Paris: International Astronomical Union, 2015. . Acesso em: 17 mar. 2026. -
APA
Soja, A. C., Sodré Júnior, L., Cypriano, E. S., & Lima Neto, G. C. B. (2015). The galaxy cluster RXC J1504-0248: a remarkable cool core near us. In Meeting Abstracts. Paris: International Astronomical Union. -
NLM
Soja AC, Sodré Júnior L, Cypriano ES, Lima Neto GCB. The galaxy cluster RXC J1504-0248: a remarkable cool core near us. Meeting Abstracts. 2015 ;[citado 2026 mar. 17 ] -
Vancouver
Soja AC, Sodré Júnior L, Cypriano ES, Lima Neto GCB. The galaxy cluster RXC J1504-0248: a remarkable cool core near us. Meeting Abstracts. 2015 ;[citado 2026 mar. 17 ] - Estrutura e populações galácticas de aglomerados do CFHTLS
- The merger history of the complex cluster Abell 1758: a combined weak lensing and spectroscopic view
- Two spectroscopically confirmed galaxy structures at z = 0.61 and 0.74 in the CFHTLS Deep 3 field
- O aglomerado de galáxias RXC J1504-0248
- A Gemini view of the galaxy cluster RXC J1504-0248: insights on the nature of the central gaseous filaments
- Structure and dynamics of the supercluster of galaxies SC0028-0005
- Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4–0.9] redshift range
- Investigating the merging cluster Abell 3376: weak lensing mass reconstruction
- Star formation efficiency in galaxy clusters
- Weak lensing and spectroscopic analysis of the nearby dissociative merging galaxy cluster Abell 3376
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
