Constraining 'H IND. 0' in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes (2012)
- Authors:
- Autor USP: LIMA, JOSÉ ADEMIR SALES DE - IAG
- Unidade: IAG
- DOI: 10.1088/1475-7516/2012/02/035
- Subjects: RAIOS X; AGLOMERADOS DE GALÁXIAS; COSMOLOGIA
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Journal of Cosmology and Astroparticle Physics
- ISSN: 1475-7516
- Volume/Número/Paginação/Ano: v. 2, p. 035/1-035/18, 2012
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
- Licença: other-oa
-
ABNT
HOLANDA, R. F. L et al. Constraining 'H IND. 0' in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes. Journal of Cosmology and Astroparticle Physics, v. 2, p. 035/1-035/18, 2012Tradução . . Disponível em: https://doi.org/10.1088/1475-7516/2012/02/035. Acesso em: 24 abr. 2024. -
APA
Holanda, R. F. L., Cunha, J. V., Marassi, L., & Lima, J. A. S. de. (2012). Constraining 'H IND. 0' in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes. Journal of Cosmology and Astroparticle Physics, 2, 035/1-035/18. doi:10.1088/1475-7516/2012/02/035 -
NLM
Holanda RFL, Cunha JV, Marassi L, Lima JAS de. Constraining 'H IND. 0' in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes [Internet]. Journal of Cosmology and Astroparticle Physics. 2012 ; 2 035/1-035/18.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1088/1475-7516/2012/02/035 -
Vancouver
Holanda RFL, Cunha JV, Marassi L, Lima JAS de. Constraining 'H IND. 0' in general dark energy models from Sunyaev-Zeldovich/X-ray technique and complementary probes [Internet]. Journal of Cosmology and Astroparticle Physics. 2012 ; 2 035/1-035/18.[citado 2024 abr. 24 ] Available from: https://doi.org/10.1088/1475-7516/2012/02/035 - Influence of a stochastic term on the meszaros effect
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- Acceleration of the Universe with Sunyaev-Zeldovich and X-ray Data from galaxy clusters
- Mass inhomogeneities and the angular size-redshift relation
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Informações sobre o DOI: 10.1088/1475-7516/2012/02/035 (Fonte: oaDOI API)
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