Can old galaxies at high redshifts and baryon acoustic oscillations constrains 'H IND. 0'? (2009)
- Authors:
- Autor USP: LIMA, JOSÉ ADEMIR SALES DE - IAG
- Unidade: IAG
- Subjects: DISTÂNCIAS ESTELARES; GALÁXIAS; ESCALAS DE DISTÂNCIAS; COSMOLOGIA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 690, n.1, p. L85-L88, 2009
-
ABNT
LIMA, José Ademir Sales de e CUNHA, J.V e JESUS, J. F. Can old galaxies at high redshifts and baryon acoustic oscillations constrains 'H IND. 0'?. The Astrophysical Journal, v. 690, n. 1, p. L85-L88, 2009Tradução . . Acesso em: 24 abr. 2024. -
APA
Lima, J. A. S. de, Cunha, J. V., & Jesus, J. F. (2009). Can old galaxies at high redshifts and baryon acoustic oscillations constrains 'H IND. 0'? The Astrophysical Journal, 690( 1), L85-L88. -
NLM
Lima JAS de, Cunha JV, Jesus JF. Can old galaxies at high redshifts and baryon acoustic oscillations constrains 'H IND. 0'? The Astrophysical Journal. 2009 ; 690( 1): L85-L88.[citado 2024 abr. 24 ] -
Vancouver
Lima JAS de, Cunha JV, Jesus JF. Can old galaxies at high redshifts and baryon acoustic oscillations constrains 'H IND. 0'? The Astrophysical Journal. 2009 ; 690( 1): L85-L88.[citado 2024 abr. 24 ] - Influence of a stochastic term on the meszaros effect
- Constraining 'H IND.0' from Sunyaev-Zel´dovich effect, galaxy clusters X-ray data, and baryon oscillations
- Análogos clássicos para cosmologias relativísticas aceleradas: uma abordagem langrangiana
- Chemical potential and the nature of the dark energy
- CDM accelerating cosmology as an alternative to the 'lâmbda'CDM model
- Creation cold dark matter cosmology (CCDM): evolution of perturbations
- Constraining the nonextensive mass function of halos from BAO, CMB and x-ray data
- Acceleration of the Universe with Sunyaev-Zeldovich and X-ray Data from galaxy clusters
- Mass inhomogeneities and the angular size-redshift relation
- On the stochastic evolution of the inflation field
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