SciELO - Scientific Electronic Library Online

 
vol.52 número2Local systematic differences in proper motions derived from 2MASS positions índice de autoresíndice de assuntospesquisa de artigos
Home Pagelista alfabética de periódicos  

Serviços Personalizados

Journal

Artigo

Indicadores

Links relacionados

  • Não possue artigos similaresSimilares em SciELO

Compartilhar


Revista mexicana de astronomía y astrofísica

versão impressa ISSN 0185-1101

Resumo

PEIMBERT, A.; PEIMBERT, M.  e  LURIDIANA, V.. The primordial helium abundance and the number of neutrino families. Rev. mex. astron. astrofis [online]. 2016, vol.52, n.2, pp.419-424. ISSN 0185-1101.

Based on observations of H II regions and on the new computations of the recombination coefficients of the He I lines by Porter el al. we obtain a primordial helium abundance by mass of YP = 0.2446 ± 0.0029. We consider thirteen sources of error for the YP determination; some of them are mainly due to systematic effects, while the rest are mainly due to statistical effects. We compare our results with other determinations of YP present in the literature. Combining our YP value with computations of primordial nucleosynthesis we find a number of neutrino species Neff = 2.90 ± 0.22, and a neutron mean life τν = 872 ± 14 s.

Palavras-chave : early universe; galaxies: abundances; galaxies: ISM; H II regions; ISM: abundances.

        · resumo em Espanhol     · texto em Inglês