Literature DB >> 22075722

Detection of pristine gas two billion years after the Big Bang.

Michele Fumagalli1, John M O'Meara, J Xavier Prochaska.   

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.

Entities:  

Year:  2011        PMID: 22075722     DOI: 10.1126/science.1213581

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  2 in total

1.  Extremely metal-poor gas at a redshift of 7.

Authors:  Robert A Simcoe; Peter W Sullivan; Kathy L Cooksey; Melodie M Kao; Michael S Matejek; Adam J Burgasser
Journal:  Nature       Date:  2012-12-06       Impact factor: 49.962

2.  Superluminous supernovae at redshifts of 2.05 and 3.90.

Authors:  Jeff Cooke; Mark Sullivan; Avishay Gal-Yam; Elizabeth J Barton; Raymond G Carlberg; Emma V Ryan-Weber; Chuck Horst; Yuuki Omori; C Gonzalo Díaz
Journal:  Nature       Date:  2012-10-31       Impact factor: 49.962

  2 in total

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