Your browser doesn't support javascript.
loading
Detection of pristine gas two billion years after the Big Bang.
Fumagalli, Michele; O'Meara, John M; Prochaska, J Xavier.
Afiliação
  • Fumagalli M; Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA, USA. mfumagalli@ucolick.org
Science ; 334(6060): 1245-9, 2011 Dec 02.
Article em En | MEDLINE | ID: mdl-22075722
ABSTRACT
In the current cosmological model, only the three lightest elements were created in the first few minutes after the Big Bang; all other elements were produced later in stars. To date, however, heavy elements have been observed in all astrophysical environments. We report the detection of two gas clouds with no discernible elements heavier than hydrogen. These systems exhibit the lowest heavy-element abundance in the early universe, and thus are potential fuel for the most metal-poor halo stars. The detection of deuterium in one system at the level predicted by primordial nucleosynthesis provides a direct confirmation of the standard cosmological model. The composition of these clouds further implies that the transport of heavy elements from galaxies to their surroundings is highly inhomogeneous.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies / Prognostic_studies Idioma: En Revista: Science Ano de publicação: 2011 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies / Prognostic_studies Idioma: En Revista: Science Ano de publicação: 2011 Tipo de documento: Article